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Sample records for asteroids digging soil

  1. Landing screw-rockets array on asteroids, digging soil and fueling engines in phase, to overcome the spin and to fly in space

    CERN Document Server

    Fargion, D

    2007-01-01

    To deflect impact-trajectory of massive km^3 and spinning asteroid by a few terrestrial radiuses one need a large momentum exchange. The dragging of huge spinning bodies in space by external engine seems difficult or impossible. Our solution is based on the landing of multi screw-rockets, powered by mini-nuclear engines, on the body, that dig a small fraction of the soil surface, to use as an exhaust propeller, ejecting it vertically in phase among themselves. Such a mass ejection increases the momentum exchange, their number redundancy guarantes the stability of the system. The soft landing of engine-unity may be easely achieved at low asteroid gravity. The engine array tuned activity, overcomes the asteroid angular velocity. Coherent turning of the jet heads increases the deflection efficiency. A procession along its surface may compensate at best the asteroid spin. A small skin-mass (about 2 10^4 tons) may be ejected by mini nuclear engines. Such prototypes may build first save galleries for humans on the ...

  2. Digging up the Dirt on Soil Safety

    Science.gov (United States)

    Roy, Ken

    2010-01-01

    Should middle school science teachers be concerned about students bringing in unknown sources of soil to work on in class as the activity suggests? The science is well intended, but is it safe? What are some possible safety issues that might be of concern in dealing with soil samples? This month's column provides several examples of unsuspecting…

  3. Dynamics of digging in wet soil

    CERN Document Server

    Jung, Sunghwan; Hosoi, A E

    2010-01-01

    Numerous animals live in, and locomote through, subsea soils. To move in a medium dominated by frictional interactions, many of these animals have adopted unique burrowing strategies. This paper presents a burrowing model inspired by the Atlantic razor clam ({\\it Ensis directus}), which uses deformations of its body to cyclically loosen and re-pack the surrounding soil in order to locally manipulate burrowing drag. The model reveals how an anisotropic body -- composed of a cylinder and sphere varying sinusoidally in size and relative displacement -- achieves unidirectional motion through a medium with variable frictional properties. This net displacement is attained even though the body kinematics are reciprocal and inertia of both the model organism and the surrounding medium are negligible. Our results indicate that body aspect ratio has a strong effect on burrowing velocity and efficiency, with a well-defined maximum for given kinematics and soil material properties.

  4. Structural Bionic Design for Digging Shovel of Cassava Harvester Considering Soil Mechanics

    Directory of Open Access Journals (Sweden)

    Shihao Liu

    2014-01-01

    Full Text Available In order to improve the working performance of cassava harvester, structural bionic design for its digging shovel was conducted. Taking the oriental mole cricket's paws as bionic prototype, a new structural bionic design method for digging shovel was established, which considers the morphology-configuration-function coupling bionic. A comprehensive performance comparison method was proposed, which is used to select the bionic design schemes. The proposed bionic design method was used to improve digging shovel structure of a digging-pulling style cassava harvester, and nine bionic-type digging shovels were obtained with considering the impact of soil mechanics. After conducting mechanical properties comparative analysis for bionic-type digging shovels, the bionic design rules were summed up, and the optimal design scheme of digging shovel was obtained through combining the proposed comprehensive performance comparison method with Analytic Hierarchy Process (AHP. Studies have shown that bionic design method not only can improve the overall mechanical properties of digging shovel, but also can help to improve the harvesting effect of cassava harvester, which provides a new idea for crops harvesting machinery's structural optimization design.

  5. Morphological adaptations for digging and climate-impacted soil properties define pocket gopher (Thomomys spp. distributions.

    Directory of Open Access Journals (Sweden)

    Ariel E Marcy

    Full Text Available Species ranges are mediated by physiology, environmental factors, and competition with other organisms. The allopatric distribution of five species of northern Californian pocket gophers (Thomomys spp. is hypothesized to result from competitive exclusion. The five species in this environmentally heterogeneous region separate into two subgenera, Thomomys or Megascapheus, which have divergent digging styles. While all pocket gophers dig with their claws, the tooth-digging adaptations of subgenus Megascapheus allow access to harder soils and climate-protected depths. In a Northern Californian locality, replacement of subgenus Thomomys with subgenus Megascapheus occurred gradually during the Pleistocene-Holocene transition. Concurrent climate change over this transition suggests that environmental factors--in addition to soil--define pocket gopher distributional limits. Here we show 1 that all pocket gophers occupy the subset of less energetically costly soils and 2 that subgenera sort by percent soil clay, bulk density, and shrink-swell capacity (a mineralogical attribute. While clay and bulk density (without major perturbations stay constant over decades to millennia, low precipitation and high temperatures can cause shrink-swell clays to crack and harden within days. The strong yet underappreciated interaction between soil and moisture on the distribution of vertebrates is rarely considered when projecting species responses to climatic change. Furthermore, increased precipitation alters the weathering processes that create shrink-swell minerals. Two projected outcomes of ongoing climate change--higher temperatures and precipitation--will dramatically impact hardness of soil with shrink-swell minerals. Current climate models do not include factors controlling soil hardness, despite its impact on all organisms that depend on a stable soil structure.

  6. Digging Soil Experiments for Micro Hydraulic Excavators based on Model Predictive Tracking Control

    Science.gov (United States)

    Tomatsu, Takumi; Nonaka, Kenichiro; Sekiguchi, Kazuma; Suzuki, Katsumasa

    2016-09-01

    Recently, the increase of burden to operators and lack of skilled operators are the issue in the work of the hydraulic excavator. These problems are expected to be improved by autonomous control. In this paper, we present experimental results of hydraulic excavators using model predictive control (MPC) which incorporates servo mechanism. MPC optimizes digging operations by the optimal control input which is calculated by predicting the future states and satisfying the constraints. However, it is difficult for MPC to cope with the reaction force from soil when a hydraulic excavator performs excavation. Servo mechanism suppresses the influence of the constant disturbance using the error integration. However, the bucket tip deviates from a specified shape by the sudden change of the disturbance. We can expect that the tracking performance is improved by combining MPC and servo mechanism. Path-tracking controls of the bucket tip are performed using the optimal control input. We apply the proposed method to the Komatsu- made micro hydraulic excavator PC01 by experiments. We show the effectiveness of the proposed method through the experiment of digging soil by comparing servo mechanism and pure MPC with the proposed method.

  7. ASTEROIDS

    Directory of Open Access Journals (Sweden)

    Željko Andreić

    2016-02-01

    Full Text Available Asteroids are the largest minor bodies in the Solar System. Nowadays they are in the research focus due to several facts about them: first, a subclass of asteroids can collide with Earth, and consequences of such a collision are dramatic. Second, they are now seen as source of materials that are becoming scarce on Earth, and they will be needed in future space constructions anyway. Third, they are holding clues about the origin and evolution of the Solar System. In this article, a short overview of current knowledge about asteroids is presented. Last, but not least, as several Croatian scientists were recently honored by naming an asteroid after them, a short overview of the naming process is given.

  8. ASTEROIDS

    OpenAIRE

    Željko Andreić

    2016-01-01

    Asteroids are the largest minor bodies in the Solar System. Nowadays they are in the research focus due to several facts about them: first, a subclass of asteroids can collide with Earth, and consequences of such a collision are dramatic. Second, they are now seen as source of materials that are becoming scarce on Earth, and they will be needed in future space constructions anyway. Third, they are holding clues about the origin and evolution of the Solar System. In this article, a short overv...

  9. Students Dig Deep in the Mystery Soil Lab: A Playful, Inquiry-Based Soil Laboratory Project

    Science.gov (United States)

    Thiet, Rachel K.

    2014-01-01

    The Mystery Soil Lab, a playful, inquiry-based laboratory project, is designed to develop students' skills of inquiry, soil analysis, and synthesis of foundational concepts in soil science and soil ecology. Student groups are given the charge to explore and identify a "Mystery Soil" collected from a unique landscape within a 10-mile…

  10. Structural Bionic Design for Digging Shovel of Cassava Harvester Considering Soil Mechanics

    OpenAIRE

    Shihao Liu; Shaojie Weng; Yulan Liao; Dongyun Zhu

    2014-01-01

    In order to improve the working performance of cassava harvester, structural bionic design for its digging shovel was conducted. Taking the oriental mole cricket's paws as bionic prototype, a new structural bionic design method for digging shovel was established, which considers the morphology-configuration-function coupling bionic. A comprehensive performance comparison method was proposed, which is used to select the bionic design schemes. The proposed bionic design method was used to impro...

  11. Soil Moisture and Excavation Behaviour in the Chaco Leaf-Cutting Ant (Atta vollenweideri): Digging Performance and Prevention of Water Inflow into the Nest

    OpenAIRE

    Steffen Pielström; Flavio Roces

    2014-01-01

    The Chaco leaf-cutting ant Atta vollenweideri is native to the clay-heavy soils of the Gran Chaco region in South America. Because of seasonal floods, colonies are regularly exposed to varying moisture across the soil profile, a factor that not only strongly influences workers' digging performance during nest building, but also determines the suitability of the soil for the rearing of the colony's symbiotic fungus. In this study, we investigated the effects of varying soil moisture on behavio...

  12. Soil moisture and excavation behaviour in the Chaco leaf-cutting ant (Atta vollenweideri: digging performance and prevention of water inflow into the nest.

    Directory of Open Access Journals (Sweden)

    Steffen Pielström

    Full Text Available The Chaco leaf-cutting ant Atta vollenweideri is native to the clay-heavy soils of the Gran Chaco region in South America. Because of seasonal floods, colonies are regularly exposed to varying moisture across the soil profile, a factor that not only strongly influences workers' digging performance during nest building, but also determines the suitability of the soil for the rearing of the colony's symbiotic fungus. In this study, we investigated the effects of varying soil moisture on behaviours associated with underground nest building in A. vollenweideri. This was done in a series of laboratory experiments using standardised, plastic clay-water mixtures with gravimetric water contents ranging from relatively brittle material to mixtures close to the liquid limit. Our experiments showed that preference and group-level digging rate increased with increasing water content, but then dropped considerably for extremely moist materials. The production of vibrational recruitment signals during digging showed, on the contrary, a slightly negative linear correlation with soil moisture. Workers formed and carried clay pellets at higher rates in moist clay, even at the highest water content tested. Hence, their weak preference and low group-level excavation rate observed for that mixture cannot be explained by any inability to work with the material. More likely, extremely high moistures may indicate locations unsuitable for nest building. To test this hypothesis, we simulated a situation in which workers excavated an upward tunnel below accumulated surface water. The ants stopped digging about 12 mm below the interface soil/water, a behaviour representing a possible adaptation to the threat of water inflow field colonies are exposed to while digging under seasonally flooded soils. Possible roles of soil water in the temporal and spatial pattern of nest growth are discussed.

  13. Determination of the correction factor for computation of the soil-digging force`s component by the multipurpose ground-digging machine

    OpenAIRE

    Koval, A. B.

    2016-01-01

    Summary.  Raising  of  problem.  Expansion  of  technical  and  technological  capabilities  and  scopes  of  using  of  longitudinal digging  excavators  are  relevant  and  economically  feasible.  There  is  a  need  for  creating  of  double  appointment  machines  for performing  excavation  in  civil  engineering  and  for  fortification  arrangement  of  positions  of  troops.  Formulation  of  the  task  of creating of radically new construction machines  is logical. These machines co...

  14. SOIL-TOOL INTERACTION AS A REVIEW FOR DIGGING OPERATION OF MINI HYDRAULIC EXCAVATOR

    OpenAIRE

    BHAVESHKUMAR P. PATEL,; DR. J. M. PRAJAPATI

    2011-01-01

    Since the late 50’s hydraulics have been the systems of choice where high force-to-weight ratios are required. Today hydraulic excavators are widely used in construction, mining, excavation, and forestryapplications. The skilled operator also cannot know about the terrain condition, soil parameters, and the soil-tool interaction forces exerted during excavation operation are required to find because these forces helpful for better design of the tool, backhoe parts and for trajectory planning....

  15. Digging the New York City Skyline: soil fungal communities in green roofs and city parks.

    Science.gov (United States)

    McGuire, Krista L; Payne, Sara G; Palmer, Matthew I; Gillikin, Caitlyn M; Keefe, Dominique; Kim, Su Jin; Gedallovich, Seren M; Discenza, Julia; Rangamannar, Ramya; Koshner, Jennifer A; Massmann, Audrey L; Orazi, Giulia; Essene, Adam; Leff, Jonathan W; Fierer, Noah

    2013-01-01

    In urban environments, green roofs provide a number of benefits, including decreased urban heat island effects and reduced energy costs for buildings. However, little research has been done on the non-plant biota associated with green roofs, which likely affect their functionality. For the current study, we evaluated whether or not green roofs planted with two native plant communities in New York City functioned as habitats for soil fungal communities, and compared fungal communities in green roof growing media to soil microbial composition in five city parks, including Central Park and the High Line. Ten replicate roofs were sampled one year after planting; three of these roofs were more intensively sampled and compared to nearby city parks. Using Illumina sequencing of the fungal ITS region we found that green roofs supported a diverse fungal community, with numerous taxa belonging to fungal groups capable of surviving in disturbed and polluted habitats. Across roofs, there was significant biogeographical clustering of fungal communities, indicating that community assembly of roof microbes across the greater New York City area is locally variable. Green roof fungal communities were compositionally distinct from city parks and only 54% of the green roof taxa were also found in the park soils. Phospholipid fatty acid analysis revealed that park soils had greater microbial biomass and higher bacterial to fungal ratios than green roof substrates. City park soils were also more enriched with heavy metals, had lower pH, and lower quantities of total bases (Ca, K, and Mg) compared to green roof substrates. While fungal communities were compositionally distinct across green roofs, they did not differentiate by plant community. Together, these results suggest that fungi living in the growing medium of green roofs may be an underestimated component of these biotic systems functioning to support some of the valued ecological services of green roofs.

  16. Digging the New York City Skyline: soil fungal communities in green roofs and city parks.

    Directory of Open Access Journals (Sweden)

    Krista L McGuire

    Full Text Available In urban environments, green roofs provide a number of benefits, including decreased urban heat island effects and reduced energy costs for buildings. However, little research has been done on the non-plant biota associated with green roofs, which likely affect their functionality. For the current study, we evaluated whether or not green roofs planted with two native plant communities in New York City functioned as habitats for soil fungal communities, and compared fungal communities in green roof growing media to soil microbial composition in five city parks, including Central Park and the High Line. Ten replicate roofs were sampled one year after planting; three of these roofs were more intensively sampled and compared to nearby city parks. Using Illumina sequencing of the fungal ITS region we found that green roofs supported a diverse fungal community, with numerous taxa belonging to fungal groups capable of surviving in disturbed and polluted habitats. Across roofs, there was significant biogeographical clustering of fungal communities, indicating that community assembly of roof microbes across the greater New York City area is locally variable. Green roof fungal communities were compositionally distinct from city parks and only 54% of the green roof taxa were also found in the park soils. Phospholipid fatty acid analysis revealed that park soils had greater microbial biomass and higher bacterial to fungal ratios than green roof substrates. City park soils were also more enriched with heavy metals, had lower pH, and lower quantities of total bases (Ca, K, and Mg compared to green roof substrates. While fungal communities were compositionally distinct across green roofs, they did not differentiate by plant community. Together, these results suggest that fungi living in the growing medium of green roofs may be an underestimated component of these biotic systems functioning to support some of the valued ecological services of green roofs.

  17. Digging the New York City Skyline: soil fungal communities in green roofs and city parks.

    Science.gov (United States)

    McGuire, Krista L; Payne, Sara G; Palmer, Matthew I; Gillikin, Caitlyn M; Keefe, Dominique; Kim, Su Jin; Gedallovich, Seren M; Discenza, Julia; Rangamannar, Ramya; Koshner, Jennifer A; Massmann, Audrey L; Orazi, Giulia; Essene, Adam; Leff, Jonathan W; Fierer, Noah

    2013-01-01

    In urban environments, green roofs provide a number of benefits, including decreased urban heat island effects and reduced energy costs for buildings. However, little research has been done on the non-plant biota associated with green roofs, which likely affect their functionality. For the current study, we evaluated whether or not green roofs planted with two native plant communities in New York City functioned as habitats for soil fungal communities, and compared fungal communities in green roof growing media to soil microbial composition in five city parks, including Central Park and the High Line. Ten replicate roofs were sampled one year after planting; three of these roofs were more intensively sampled and compared to nearby city parks. Using Illumina sequencing of the fungal ITS region we found that green roofs supported a diverse fungal community, with numerous taxa belonging to fungal groups capable of surviving in disturbed and polluted habitats. Across roofs, there was significant biogeographical clustering of fungal communities, indicating that community assembly of roof microbes across the greater New York City area is locally variable. Green roof fungal communities were compositionally distinct from city parks and only 54% of the green roof taxa were also found in the park soils. Phospholipid fatty acid analysis revealed that park soils had greater microbial biomass and higher bacterial to fungal ratios than green roof substrates. City park soils were also more enriched with heavy metals, had lower pH, and lower quantities of total bases (Ca, K, and Mg) compared to green roof substrates. While fungal communities were compositionally distinct across green roofs, they did not differentiate by plant community. Together, these results suggest that fungi living in the growing medium of green roofs may be an underestimated component of these biotic systems functioning to support some of the valued ecological services of green roofs. PMID:23469260

  18. Digging the New York City Skyline: Soil Fungal Communities in Green Roofs and City Parks

    OpenAIRE

    McGuire, Krista L.; Payne, Sara G.; Palmer, Matthew I; Gillikin, Caitlyn M.; Dominique Keefe; Su Jin Kim; Gedallovich, Seren M.; Julia Discenza; Ramya Rangamannar; Koshner, Jennifer A.; Audrey L Massmann; Giulia Orazi; Adam Essene; Leff, Jonathan W.; Noah Fierer

    2013-01-01

    In urban environments, green roofs provide a number of benefits, including decreased urban heat island effects and reduced energy costs for buildings. However, little research has been done on the non-plant biota associated with green roofs, which likely affect their functionality. For the current study, we evaluated whether or not green roofs planted with two native plant communities in New York City functioned as habitats for soil fungal communities, and compared fungal communities in green...

  19. Effect of mole (Talpaеuropаеa digging activity on soil microflora in case of soil cadmium pollution

    Directory of Open Access Journals (Sweden)

    O. Y. Pakhomov

    2006-01-01

    Full Text Available Influence of fossorial activity of European mole Talpa еuropаеа on number and distribution of soil microorganisms under conditions of cadmium pollution of the soil is characterized. Mammals’ fossorial activity is an important natural ecological factor that contributes to microflora rehabilitation and development under conditions of contamination.

  20. Kidnapping small icy asteroids in Earth near encounter to harbour life and to deflect trajectory

    Science.gov (United States)

    Fargion, Daniele

    2016-07-01

    The inter-planetary flight for human being is under danger because of unscreened and lethal solar flare radioactive showers. The screening of the astronauts by huge superconducting magnetic fields is unrealistic by many reasons. On the contrary the ability to reach nearby icy asteroids, to harbour there a complete undergound room where ecological life systems are first set, this goal may offer a later natural and safe currier for future human stations and enterprise. The need to deflect such a small size (a few thousands tons objects) maybe achieved by micro nuclear engines able to dig the asteroid icy skin, to heat and propel the soil by a synchronous jet engine array, bending and driving it to any desired trajectories. The need for such a wide collection of icy asteroid stations, often in a robotic ibernated state, it will offer the safe help station, raft in the wide space sea, where to collect material or energy in long human planetary travels.

  1. Asteroid thermophysical modeling

    CERN Document Server

    Delbo, Marco; Emery, Joshua P; Rozitis, Ben; Capria, Maria Teresa

    2015-01-01

    The field of asteroid thermophysical modeling has experienced an extraordinary growth in the last ten years, as new thermal infrared data became available for hundreds of thousands of asteroids. The infrared emission of asteroids depends on the body's size, shape, albedo, thermal inertia, roughness and rotational properties. These parameters can therefore be derived by thermophysical modeling of infrared data. Thermophysical modeling led to asteroid size estimates that were confirmed at the few-percent level by later spacecraft visits. We discuss how instrumentation advances now allow mid-infrared interferometric observations as well as high-accuracy spectro-photometry, posing their own set of thermal-modeling challenges.We present major breakthroughs achieved in studies of the thermal inertia, a sensitive indicator for the nature of asteroids soils, allowing us, for instance, to determine the grain size of asteroidal regoliths. Thermal inertia also governs non-gravitational effects on asteroid orbits, requir...

  2. Test dig selv!

    DEFF Research Database (Denmark)

    Hølge-Hazelton, Bibi; Nielsen, Gregers; Langstrup, Henriette;

    2011-01-01

    Teknologirådet omkring rapporten ”Test dig selv! – Vurderinger og anbefalinger vedrørende anvendelse medicinsk udstyr til selvtestning. Offentliggjort d. 25.10.11.......Teknologirådet omkring rapporten ”Test dig selv! – Vurderinger og anbefalinger vedrørende anvendelse medicinsk udstyr til selvtestning. Offentliggjort d. 25.10.11....

  3. Digging of 'Snow White' Begins

    Science.gov (United States)

    2008-01-01

    NASA's Phoenix Mars Lander began excavating a new trench, dubbed 'Snow White,' in a patch of Martian soil located near the center of a polygonal surface feature, nicknamed 'Cheshire Cat.' The trench is about 2 centimeters (.8 inches) deep and 30 centimeters (about 12 inches) long. The 'dump pile' is located at the top of the trench, the side farthest away from the lander, and has been dubbed 'Croquet Ground.' The digging site has been named 'Wonderland.' At this early stage of digging, the Phoenix team did not expect to find any of the white material seen in the first trench, now called 'Dodo-Goldilocks.' That trench showed white material at a depth of about 5 centimeters (2 inches). More digging of Snow White is planned for coming sols, or Martian days. The dark portion of this image is the shadow of the lander's solar panel; the bright areas within this region are not in shadow. Snow White was dug on Sol 22 (June 17, 2008) with Phoenix's Robotic Arm. This picture was acquired on the same day by the lander's Surface Stereo Imager. This image has been enhanced to brighten shaded areas. The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

  4. Digging Movie from Phoenix's Sol 18

    Science.gov (United States)

    2008-01-01

    The Surface Stereo Imager on NASA's Phoenix Mars Lander recorded the images combined into this movie of the lander's Robotic Arm enlarging and combining the two trenches informally named 'Dodo' (left) and 'Goldilocks.' The 21 images in this sequence were taken over a period of about 2 hours during Phoenix's Sol 18 (June 13, 2008), or the 18th Martian day since landing. The main purpose of the Sol 18 dig was to dig deeper for learning the depth of a hard underlying layer. A bright layer, possibly ice, was increasingly exposed as the digging progressed. Further digging and scraping in the combined Dodo-Goldilocks trench was planned for subsequent sols. The combined trench is about 20 centimeters (about 8 inches) wide. The depth at the end of the Sol 18 digging is 5 to 6 centimeters (about 2 inches). The Goldilocks trench was the source of soil samples 'Baby Bear' and 'Mama Bear,' which were collected on earlier sols and delivered to instruments on the lander deck. The Dodo trench was originally dug for practice in collecting and depositing soil samples. The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

  5. Sequential Soil Transport and Its Influence on the Spatial Organisation of Collective Digging in Leaf-Cutting Ants

    OpenAIRE

    Steffen Pielström; Flavio Roces

    2013-01-01

    The Chaco leaf-cutting ant Atta vollenweideri (Forel) inhabits large and deep subterranean nests composed of a large number of fungus and refuse chambers. The ants dispose of the excavated soil by forming small pellets that are carried to the surface. For ants in general, the organisation of underground soil transport during nest building remains completely unknown. In the laboratory, we investigated how soil pellets are formed and transported, and whether their occurrence influences the spat...

  6. DigDag

    DEFF Research Database (Denmark)

    Knudsen, Bo Nissen

    each archive, or archival system. The DigDag project establishes a uniform research infrastructure through a webGIS within history, archaeology, place-names, statistics and geography: a digital cartographical skeleton for thematic mapping and analysis which will generate new interdisciplinary research...

  7. Digging One's Own Grave

    Directory of Open Access Journals (Sweden)

    Arvo Krikmann

    2007-01-01

    Full Text Available The paper aims to demonstrate that some points in the explicationof the figurative expression digging one’s own grave via the concept of blending given by Gilles Fauconnier and Mark Turner are problematic: (1 Not understanding the consequences of one’s deeds is an almost universal presuppositionof and impulse or motivation for actualizing any utterance with a forewarning or gloating content (e.g., proverbs, not the singularity characterizing just the expression of grave-digging as such. (2 The inversion of causal and temporal structure is not the case because of metonymic association between the concepts of the grave and death, as a result of which specific causal and temporal order loses any significance. Many synonymous examples can be given in which the image refers to events before the death, between the death and funeral, as well as those after burial. (3 The source domain needs not to be restricted to natural death and modern civilized funerals but should include also the cases of violent deaths, e.g., the scenario of execution and the scenario of hunting and trapping. Preliminarily, a very brief synopsis of the main phases of development of cognitive linguistic theory of metaphor and some favourite examples of blends, used also in previous works, is provided.

  8. Microchemical and Structural Evidence for Space Weathering in Soils from Asteroid Itokawa

    Science.gov (United States)

    Thompson, M. S.; Christoffersen, R.; Zega, T. J.

    2013-01-01

    The chemistry, microstructure and optical properties of grains on the surfaces of airless bodies are continu-ously modified due to their interactions predominantly with solar energetic ions and micrometeorite impacts. Collectively known as space weathering, this phenomenon results in a discrepancy between remotely sensed spectra from asteroids and those ac-quired directly from meteorites. The return of pristine samples from the asteroid Itokawa provides insight into surface processes on airless bodies and will help in correlating remote sensing data with laboratory analysis of meteorites. Samples and Methods: We examined Itokawa samples RA-QD02-0042-01 and RA-QD-02-0042-02, ultramicrotomed sec-tions of a singular grain prepared by the Hayabusa sample cura-tion team. We analyzed these slices using a 200 keV JEOL 2010F transmission electron microscope (TEM) at Arizona State Uni-versity and a 200 keV JEOL 2500SE TEM at NASA JSC. Both field emission TEMs are equipped with energy-dispersive X-ray spectrometers (EDS) and scanning TEM (STEM) detectors. Results and Discussion: TEM observations reveal that the sectioned grain predominantly consists of a single crystal of low-Ca orthopyroxene, with subsidiary smaller regions of olivine, Fe-Ni sulfide, and Fe-Ni metal. EDS-spectrum imaging and high-resolution TEM (HRTEM) show local, nanocrystalline regions of the outermost 2 to 5 nm of the pyroxene are composed of an Fe-Mg-S-rich and Si- and O-depleted layer that is underlain by a 2- to 5-nm thick amorphous zone enriched in Si. These layers occur in multiple microtome slices and have uniform thicknesses. We also observe localized 'islands' of material on the surface of the pyroxene which HRTEM imaging indicates are amorphous and EDS measurements show are compositionally heterogeneous. A 10- to 60-nm thick partially amorphous zone occurs below the compositionally distinct rim. While this this zone is associated with the compositionally heterogeneous outer layer, it also occurs

  9. Dig-face monitoring during excavation of a radioactive plume at Mound Laboratory, Ohio

    International Nuclear Information System (INIS)

    A dig-face monitoring system consists of onsite hardware for collecting information on changing chemical, radiological, and physical conditions in the subsurface soil during the hazardous site excavation. A prototype dig-face system was take to Mount Laboratory for a first trial. Mound Area 7 was the site of historical disposals of 232Th, 227Ac, and assorted debris. The system was used to monitor a deep excavation aimed at removing 227Ac-contaminated soils. Radiological, geophysical, and topographic sensors were used to scan across the excavation dig-face at four successive depths as soil was removed. A 3-D image of the contamination plumes was developed; the radiation sensor data indicated that only a small portion of the excavated soil volume was contaminated. The spatial information produced by the dig-face system was used to direct the excavation activities into the area containing the 227Ac and to evaluate options for handling the separate 232Th plume

  10. Asteroid taxonomy

    Science.gov (United States)

    Tholen, David J.; Barucci, M. Antonietta

    1989-01-01

    The spectral reflectivity of asteroid surfaces over the wavelength range of 0.3 to 1.1 micron can be used to classify these objects into several broad groups with similar spectral characteristics. The three most recently developed taxonomies group the asteroids into 9, 11, or 14 different clases, depending on the technique used to perform the analysis. The distribution of the taxonomic classes shows that darker and redder objects become more dominant at larger heliocentric distances, while the rare asteroid types are found more frequently among the small objects of the planet-crossing population.

  11. Black-footed ferret digging activity in summer

    Science.gov (United States)

    Eads, David A.; Biggins, Dean E.; Marsh, Dustin; Millspaugh, Joshua J.; Livieri, Travis M.

    2012-01-01

    Black-footed ferrets (Mustela nigripes) excavate soil from prairie dog (Cynomys spp.) burrows, thereby creating characteristic soil deposits at burrow openings. These soil deposits have been observed only rarely in summer. We monitored adult ferrets during June–October of the years 2007 and 2008 on a 452-ha colony of black-tailed prairie dogs (Cynomys ludovicianus) in the Conata Basin, South Dakota. We located and identified ferret excavations during nighttime spotlight surveys for ferrets and daytime sampling of prairie dog burrow openings around locations where ferrets were located via spotlight. We accumulated 48 observations of in-process or recently completed ferret excavations during spotlight surveys (21 in 2007, 27 in 2008) and located 51 diggings during daytime burrow sampling (25 in 2007, 26 in 2008). We located diggings during 5.5% of spotlight observations, most frequently in July–August. These results collectively suggest ferrets may frequently excavate soil in summer, because prairie dogs frequently use soil to plug burrow openings and tunnels in defense against ferrets. Prairie dogs might frequently destroy soil deposits left by ferrets during summer, thereby reducing detection of diggings by biologists.

  12. It is not all pheromones: No evidence that pheromones affect digging face choice during ant nest excavation.

    Science.gov (United States)

    Bruce, Andrew I

    2016-01-01

    Ants create nests of a size that is tailored to the number of individuals in a nest via a self-organized process. It is not yet clear how they accomplish this. Deposition and evaporation of pheromones at the digging face has been hypothesised by Deneubourg and Franks (1995) and Buhl et al. (2005) to be part of the nest construction process, with models being presented to support this contention. This hypothesis was tested by allowing groups of 5 Acromyrmex lundi workers to choose between two excavation sites, one that was freshly exposed to digging and one where digging had ceased an hour previously. It was expected that if pheromones played a role in stimulating digging, then ants would show a preference for digging in the "fresh" sites rather than the "aged" sites where the putative digging pheromone had decayed. No significant difference in digging activity between "fresh" and "aged" sites was detected. It is therefore likely that, while digging pheromones may play other roles in other parts of the digging system, they do not play an important role in regulation of soil excavation at the digging face. PMID:26529291

  13. Careful where you dig

    International Nuclear Information System (INIS)

    Improved excavation techniques help contractors at former nuclear weapons site avoid digging up the past. The Department of Energy's Hanford Site is an excavator's nightmare. It's one of the country's oldest nuclear sites, with facilities that were built in the rush to win a world war and then a decades-long arms race. During World War II the reactors and process facilities at Hanford were constructed with utmost secrecy. For instance, the site was divided up into various, distinct processing areas -- each with its own separate survey coordinate system to confuse an invading enemy. In 1989 when the Cold War ended, Hanford began its metamorphosis from top secret defense site to the nation's largest and most complex nuclear waste cleanup project. National defense urgency and past environmental and as-built standards of the time left a legacy of chemical discharges and semi-hidden utilities. Also, the new cleanup mission included a new interest in privatization and outsourcing for engineering and services. This brought an influx of new contractors and personnel with no work experience of the Hanford Site. In the 50-year history of Hanford, various government agencies, contractors and their policies have come and gone. As federal budgets rose and fell, so did the accuracy of as-built documentation. At one point, jobs below$150,000 in value were not even documented as they were built because it wasn't considered cost-effective. Many utilities were field-routed, leaving no dependable as-built drawings. To be cost-effective, adjacent construction projects often shared a common excavation, both adding underground lines to the same trench. This 1ed to mixed confidence levels in the accuracy of the as-builts

  14. Asteroids IV

    Science.gov (United States)

    Michel, Patrick; DeMeo, Francesca E.; Bottke, William F.

    Asteroids are fascinating worlds. Considered the building blocks of our planets, many of the authors of this book have devoted their scientific careers to exploring them with the tools of our trade: ground- and spacebased observations, in situ space missions, and studies that run the gamut from theoretical modeling efforts to laboratory work. Like fossils for paleontologists, or DNA for geneticists, they allow us to construct a veritable time machine and provide us with tantalizing glimpses of the earliest nature of our solar system. By investigating them, we can probe what our home system was like before life or even the planets existed. The origin and evolution of life on our planet is also intertwined with asteroids in a different way. It is believed that impacts on the primordial Earth may have delivered the basic components for life, with biology favoring attributes that could more easily survive the aftermath of such energetic events. In this fashion, asteroids may have banished many probable avenues for life to relative obscurity. Similarly, they may have also prevented our biosphere from becoming more complex until more recent eras. The full tale of asteroid impacts on the history of our world, and how human life managed to emerge from myriad possibilities, has yet to be fully told. The hazard posed by asteroid impacts to our civilization is low but singular. The design of efficient mitigation strategies strongly relies on asteroid detection by our ground- and spacebased surveys as well as knowledge of their physical properties. A more positive motivation for asteroid discovery is that the proximity of some asteroids to Earth may allow future astronauts to harvest their water and rare mineral resources for use in exploration. A key goal of asteroid science is therefore to learn how humans and robotic probes can interact with asteroids (and extract their materials) in an efficient way. We expect that these adventures may be commonplace in the future

  15. Energetic cost of digging behavior in workers of the leaf-cutting ant Atta sexdens (Fabricius)

    OpenAIRE

    Roberto da Silva Camargo; Juliane F. S. Lopes; Luiz Carlos Forti

    2013-01-01

    Energetic cost of digging behavior in workers of the leaf-cutting ant Atta sexdens (Fabricius). During nest excavation, leaf-cutting ant workers undergo reduction in their body reserve, particularly carbohydrates. In order to estimate the energetic cost of digging, groups of 30 workers of the leaf-cutting ant Atta sexdens were sealed in a hermetic chamber for 24, 48 and 72 hours, with and without soil for digging, and had the CO2 concentration measured using respirometric chambers as well as ...

  16. Digging Up Local History | Poster

    Science.gov (United States)

    By Carolynne Keenan, Contributing Writer In the beginning weeks of summer, Recreation and Welfare (R&W) Club Frederick members experienced a once-in-a-lifetime activity: an archaeological dig in Walkersville, alongside Charlie Hall, Ph.D., Maryland state terrestrial archaeologist.

  17. Digging for knowledge

    Science.gov (United States)

    Szu, Harold; Jenkins, Jeffrey; Hsu, Charles; Goehl, Steve; Miao, Liden; Cader, Masud; Benachenhou, Dalila

    2009-04-01

    The "smile of a mother" is always recognized, whenever and wherever. But why is my PC always dumb and unable to recognize me or my needs, whoever or whatever? This paper postulates that such a 6 W's query and search system needs matching storage. Such a lament will soon be mended with a smarter PC, or a smarter Google engine, a network computer, working in the field of data retrieval, feature extraction, reduction, and knowledge precipitation. Specifically, the strategy of modern information storage and retrieval shall work like our brains, which are constantly overwhelmed by 5 pairs of identical tapes taken by eyes, ears, etc. 5 high fidelity sensors generate 5 pairs of high definition tapes which produce the seeing and hearing etc. in our perception. This amounts to 10 tapes recorded in a non-abridged fashion. How can we store and retrieve them when we need to? We must reduce the redundancy, enhancing the signal noise ratio, and fusing invariant features using a simple set of mathematical operations to write according to the union and read by the intersection in the higher dimensional vector space. For example, (see paper for equation) where the query must be phrased in terms of the union of imprecise or partial set of 6w's denoted by the union of lower case w's. The upper case W's are the archival storage of a primer tree. A simplified humanistic representation may be called the 6W space (who, what, where, when, why, how), also referred to as the Newspaper geometry. It seems like mapping the 6W to the 3W (World Wide Web) is becoming relatively easier. It may thus become efficient and robust by rapidly digging for knowledge through the set operations of union, writing, and intersection, reading, upon the design of 6 W query searching engine matched efficiently by the 6W vector index databases. In fact, Newspaper 6D geometry may be reduced furthermore by PCA (Principal Component Analysis) eigenvector mathematics and mapped into the 2D causality space comprised of

  18. Search for Asteroid-Asteroid Encounters

    Directory of Open Access Journals (Sweden)

    Luis A. Mammana

    2001-01-01

    Full Text Available Earlier studies about asteroids did not consider mutual interactions since they assume a negligible asteroid mass. In 1966 Hertz took into account for the first time the gravitational effects produced by an asteroid on another for mass determination. This gravitational action becomes relevant for enough effective encounters. The most efficient gravitational interaction is that produced in a large time interval and for small distances. For each particular caseful it is relevant to perform a care analysis in order to determinate the feasibility in the mass determination and improved orbital elements. In the present paper we performed a search of asteroid-asteroid encounters occurred in the twenty century for the first 3000 numbered asteroids . Of all encounters we have selected only those asteroid pairs in which one of the asteroids has a diameter larger than 200 km and the other one (the smaller an observational interval of at least ten years.

  19. Flyght Dynamics of Artificial Satellite of the Minor Asteroid

    Science.gov (United States)

    Zakharov, Alexander; Eismont, Natan; Ledkov, Anton; Simonov, Alexander; Pol, Vadim

    During last years the scientific interest to the asteroid is constantly growing. It may be explained by different reasons. One of the most important from them is confirmation of the fact that the asteroids present the real hazard to the Earth. The Chelyabinsk event demonstrates strong in support of this statement. Besides, the asteroids exploration promises to supply new data for understanding of the solar system origin and evolution. And the projects aimed to reach this goal have begun from the NASA NEAR mission to Eros. It was the first one when the spacecraft was landed on the surface of the asteroid. The other successive mission was fulfilled by JAXA with Hayabusa spacecraft which has returned to the Earth soil samples of Itokawa asteroid. In the nearest future the mission to RQ 36 asteroid is planned supposing landing and soil samples return. Unavoidable phase of such missions is the spacecraft flight in vicinity of the target asteroid, for example on the asteroid satellite orbit. It should be mentioned that quite visible number of asteroids has geometric form which is far from being sphere. Accordingly the gravity field of such asteroid cannot be presented as the one close to sphere. The problem is that prior to the mission to the asteroid one cannot receive good enough knowledge of its gravity field and even its gravity field constant. In the paper the flight dynamics problem of spacecraft moving along asteroid satellite orbit is explored. It is supposed that the asteroid is comparatively small with diameter (maximum size) about 300 m, like Apophis asteroid has, or less. To approximate the gravity field of asteroid the last is considered as totality of mass points. We assume such approach as more simple and effective as compared with the commonly accepted use of Legendre polynomial expansion. Different orbits near asteroid are analyzed with the sets of orbital parameters determining the size of orbit, its shape and position with respect to the Sun. The goal

  20. Asteroid rotation rates

    Science.gov (United States)

    Dermott, S. F.; Harris, A. W.; Murray, C. D.

    1984-01-01

    A trend of increasing mean rotational frequency with increasing diameter is noted in asteroids with diameters greater than 120 km, irrespective of M-, S-, and C-type asteroid subset and family or nonfamily membership. This trend cannot be accounted for by observational selection. For asteroids with diameters smaller than 120 km mean rotational frequency increases with decreasing diameter, but within this group there is a subset with exceptionally long rotational periods. This marked change in the distribution at 120-km diameter could separate primordial asteroids from their collision products. It is also noted that, for asteroids of a given diameter, M asteroids rotate faster than S asteroids, which in turn rotate faster than C asteroids. For all types, family members rotate faster than nonfamily members.

  1. The Active Asteroids

    CERN Document Server

    Jewitt, David; Agarwal, Jessica

    2015-01-01

    Some asteroids eject dust, producing transient, comet-like comae and tails; these are the active asteroids. The causes of activity in this newly-identified population are many and varied. They include impact ejection and disruption, rotational instabilities, electrostatic repulsion, radiation pressure sweeping, dehydration stresses and thermal fracture, in addition to the sublimation of asteroidal ice. These processes were either unsuspected or thought to lie beyond the realm of observation before the discovery of asteroid activity. Scientific interest in the active asteroids lies in their promise to open new avenues into the direct study of asteroid destruction, the production of interplanetary debris, the abundance of asteroid ice and the origin of terrestrial planet volatiles.

  2. Digging Deeper: Looking Beyond Behavior to Discover Meaning

    Medline Plus

    Full Text Available ... Email Client Print Español Digging Deeper: Looking Beyond Behavior to Discover Meaning A Unit of Four Online Lessons Digging Deeper: Looking Beyond Behavior to Discover Meaning is a unit of four ...

  3. Digging Deeper: Looking Beyond Behavior to Discover Meaning

    Medline Plus

    Full Text Available ... Digging Deeper: Looking Beyond Behavior to Discover Meaning A Unit of Four Online Lessons Digging Deeper: Looking Beyond Behavior to Discover Meaning is a unit of four lessons that explore and apply ...

  4. The asteroid ring

    Science.gov (United States)

    Dermott, S. F.; Murray, C. D.

    1982-01-01

    From a statistical analysis of asteroid orbital period data, it is shown that the present distribution of asteroids is strongly correlated with the present orbital period of Jupiter (to 1 part in 5000). By analyzing the distribution of orbital eccentricities and inclinations it is shown that the resonant structure of the belt was formed after the asteroids dispersed from the near-coplanar disk in which they accreted.

  5. An overview of the asteroids

    Science.gov (United States)

    Binzel, Richard P.

    1989-01-01

    An introductory overview of the field of asteroid science is presented, with emphasis placed on the accomplishments of the 1980s. Following the survey of known asteroids, attention is given to the observations of asteroids with the IRAS. Particular consideration is given to the origin and evolution of asteroids and their interrelations. Possible future directions of asteroid research are discussed together with the potential of the Hubble Space Telescope for providing new data on asteroid surface chemistry, geology, structure, and morphology.

  6. Effect of Ni on aspartataminotransferase activity in Glechoma hederacea leaves subject to digging function by mammals

    Directory of Open Access Journals (Sweden)

    O. Y. Pakhomov

    2013-10-01

    Full Text Available Using simple and highly sensitive methods of biochemical analysis (determination of total enzyme activity of the class transferase and content of water-soluble protein fraction in Glechoma hederacea L. leaves, as response mechanisms of organisms to environmental change we have detected an environment forming role played by Talpa europaea L. (european mole, through its digging function, studied against the background of anthropogenic Ni pollution with concentrations of 0.2, 1.0 and 2.0 g/m2, which was equivalent to the presence of Ni at 1, 5, 10 times the dose of maximum permissible concentration (MPC. Thus, we discovered the fact of the reduction in total activity of aspartat­aminotransferase (AST in G. hederacea leaves by 12–65% and concentrations of water-soluble protein fraction by 30–60% relative to control (the area without pollution of Ni and digging activity of mammals. The combined effect of the digging activity of T. europaea and Ni at doses of 5, 10 MAC contributed to the increased activity of the enzyme from 2.3 to 3.0 times (compared with the control in the corresponding concentration Ni. The concentration of water soluble protein fraction under the combined effect of the digging activity and Ni at maximum concentration in G. hederacea leaves was reduced by 2 times (compared with the control in the corresponding concentration Ni, because it was difficult for the system to operate the mechanisms of recovery and normalization function, while at low and medium metal concentration the processes of protein metabolism increased by 11–150%. Вesides, the іnfluence of the digging activity of mammals (Apodemus sylvaticus L., A. flavicollis Melchior, Clethrionomys glareoles Schreber as our examples under the condition of artificial Ni soil pollution of the Ni polluted soil in the natural humid forest was assessed. Pollutants drastically influence the proteolityc activity of the soil that reflects microorganism’s metabolism. The

  7. Energetic cost of digging behavior in workers of the leaf-cutting ant Atta sexdens (Fabricius

    Directory of Open Access Journals (Sweden)

    Roberto da Silva Camargo

    2013-12-01

    Full Text Available Energetic cost of digging behavior in workers of the leaf-cutting ant Atta sexdens (Fabricius. During nest excavation, leaf-cutting ant workers undergo reduction in their body reserve, particularly carbohydrates. In order to estimate the energetic cost of digging, groups of 30 workers of the leaf-cutting ant Atta sexdens were sealed in a hermetic chamber for 24, 48 and 72 hours, with and without soil for digging, and had the CO2 concentration measured using respirometric chambers as well as volume of soil excavated (g. As expected, the worker groups that carried out soil excavation expelled more carbon dioxide than the groups that did not excavate. Therefore, a worker with body mass of 9.65 ± 1.50 mg dug in average 0.85 ± 0.27 g of soil for 24 hours, consuming ca. 0.58 ± 0.23 J. In this study, we calculate that the energetic cost of excavation per worker per day in the experimental set-up was ca. 0.58 J.

  8. Modeling of Asteroid Shapes

    CERN Document Server

    Kokorev, Andrii

    2016-01-01

    In this article we consider different methods of modeling asteroid shapes, especially lightcurve inversion technique, and scattering laws used for it. We also introduce our program, which constructs lightcurves for a given asteroid shape model. It can be used to comparing shape model with observational data.

  9. Global Asteroid Risk Analysis

    CERN Document Server

    Rumpf, Clemens

    2014-01-01

    Potentially impacting asteroids were analysed for their impact risk on the Earth. To this end, the Asteroid Risk Mitigation Optimization and Research (ARMOR) tool is currently being developed. The tool's modules are described and their validation is documented. Based on the asteroid ephemeris, the tool calculates the impact location probability distribution on the surface of the Earth (in the literature, occasionally referred to as risk corridor). NASA's Near Earth Object (NEO) risk list served as the source for asteroid ephemerides. The Line of Variation (LOV) method was employed to find virtual impactors. While offering a simple and fast way of identifying virtual impactors, the method provides a low impactor identification rate. This is because the search space is tightly constricted to the LOV and thus excludes virtual impactors located elsewhere in the asteroid position uncertainty region. The method's performance was evaluated and suggestions for improvements are provided. Application of the tool showed...

  10. Polarimetric properties of asteroids

    Science.gov (United States)

    Shestopalov, D. I.; Golubeva, L. F.

    2015-11-01

    Quite frequently astronomic polarimetric observations of different celestial bodies do not guarantee a proper phase angle coverage that is required for estimating all of the attributes of their polarization phase curves with a high accuracy. To approximate the phase dependences of polarization observed for particulate surfaces, we use a simple empiric formula recently suggested by Shestopalov (2004). The efficiency of the approximating function in a wide range of phase angles is illustrated with the use of the results of polarimetric measurements of lunar areas, lunar samples, and near-Earth asteroids. For asteroids of various types, we can reproduce their negative polarization branches with adequate accuracy and roughly estimate a probable value of the maximum polarization degree at an appropriate phase angle. From the polarimetric database available at NASA PDS [Asteroid Polarimetric Database V7.0 (2012)] we calculated the main parameters of 153 polarimetric curves of asteroids in various spectral bands with the accuracy comparable to the observation errors. One more purpose of our analysis was to find correlations between the polarimetric and photometric properties of asteroids. For C-, M-, S-, E-type asteroids, the characteristics of the negative branch of polarization curves turned out to correlate closely with the phase coefficient of the photometric function of asteroids and the photometric roughness of asteroid surfaces. This implies that the complex geometry of the surface microrelief affects the polarization properties of asteroids. In particular, the data scattering around regression lines on the plots of the albedo versus the depth of negative polarization branch and the slope of the polarimetric function at inversion angle strongly depends on the differences in the photometric roughness of asteroid surfaces.

  11. Quantitative measures for assessment of the hydraulic excavator digging efficiency

    Institute of Scientific and Technical Information of China (English)

    Dragoslav JANOSEVIC; Rosen MITREV; Boban ANDJELKOVIC; Plamen PETROV

    2012-01-01

    In this paper,quantitative measures for the assessment of the hydraulic excavator digging efficiency are proposed and developed.The following factors are considered: (a) boundary digging forces allowed for by the stability of an excavator,(b) boundary digging forces enabled by the driving mechanisms of the excavator,(c) factors taking into consideration the digging position in the working range of an excavator,and (d) sign and direction of potential digging resistive force.A corrected digging force is defined and a mathematical model of kinematic chain and drive mechanisms of a five-member excavator configuration was developed comprising: an undercarriage,a rotational platform and an attachment with boom,stick,and bucket.On the basis of the mathematical model of the excavator,software was developed for computation and detailed analysis of the digging forces in the entire workspace of the excavator.By using the developed software,the analysis of boundary digging forces is conducted and the corrected digging force is determined for two models of hydraulic excavators of the same mass (around 17000 kg) with identical kinematic chain parameters but with different parameters of manipulator driving mechanisms.The results of the analysis show that the proposed set of quantitative measures can be used for assessment of the digging efficiency of existing excavator models and to serve as an optimization criterion in the synthesis of manipulator driving mechanisms of new excavator models.

  12. Dig-event: let's socialize around events

    OpenAIRE

    Zhao, Zhenzhen; Liu, Ji; Crespi, Noel

    2012-01-01

    International audience Traditional social networks socialize around the contents that have uploaded to these sites and discover interesting contents uploaded by others. In this demo we aim to explore the idea of activity-oriented social networks. We design a novel social networking site called Dig-Event (Do-it-together Event), where people are able to share events through calendar, while discover interesting events shared by others. Our demo has been inspired by previous research on calend...

  13. Space weathering of asteroids

    CERN Document Server

    Shestopalov, D I; Cloutis, E A

    2012-01-01

    Analysis of laboratory experiments simulating space weathering optical effects on atmosphereless planetary bodies reveals that the time needed to alter the spectrum of an ordinary chondrite meteorite to resemble the overall spectral shape and slope of an S-type asteroid is about ~ 0.1 Myr. The time required to reduce the visible albedo of samples to ~ 0.05 is ~ 1 Myr. Since both these timescales are much less than the average collisional lifetime of asteroids larger than several kilometers in size, numerous low-albedo asteroids having reddish spectra with subdued absorption bands should be observed instead of an S-type dominated population. It is not the case because asteroid surfaces cannot be considered as undisturbed, unlike laboratory samples. We have estimated the number of collisions occurring in the time of 105 yr between asteroids and projectiles of various sizes and show that impact-activated motions of regolith particles counteract the progress of optical maturation of asteroid surfaces. Continual r...

  14. Asteroids - NeoWs API

    Data.gov (United States)

    National Aeronautics and Space Administration — NeoWs (Near Earth Object Web Service) is a RESTful web service for near earth Asteroid information. With NeoWs a user can: search for Asteroids based on their...

  15. The Asteroid Impact Mission

    Science.gov (United States)

    Carnelli, Ian; Galvez, Andres; Mellab, Karim

    2016-04-01

    The Asteroid Impact Mission (AIM) is a small and innovative mission of opportunity, currently under study at ESA, intending to demonstrate new technologies for future deep-space missions while addressing planetary defense objectives and performing for the first time detailed investigations of a binary asteroid system. It leverages on a unique opportunity provided by asteroid 65803 Didymos, set for an Earth close-encounter in October 2022, to achieve a fast mission return in only two years after launch in October/November 2020. AIM is also ESA's contribution to an international cooperation between ESA and NASA called Asteroid Impact Deflection Assessment (AIDA), consisting of two mission elements: the NASA Double Asteroid Redirection Test (DART) mission and the AIM rendezvous spacecraft. The primary goals of AIDA are to test our ability to perform a spacecraft impact on a near-Earth asteroid and to measure and characterize the deflection caused by the impact. The two mission components of AIDA, DART and AIM, are each independently valuable but when combined they provide a greatly increased scientific return. The DART hypervelocity impact on the secondary asteroid will alter the binary orbit period, which will also be measured by means of lightcurves observations from Earth-based telescopes. AIM instead will perform before and after detailed characterization shedding light on the dependence of the momentum transfer on the asteroid's bulk density, porosity, surface and internal properties. AIM will gather data describing the fragmentation and restructuring processes as well as the ejection of material, and relate them to parameters that can only be available from ground-based observations. Collisional events are of great importance in the formation and evolution of planetary systems, own Solar System and planetary rings. The AIDA scenario will provide a unique opportunity to observe a collision event directly in space, and simultaneously from ground-based optical and

  16. Threat Mitigation: The Asteroid Tugboat

    OpenAIRE

    Schweickart, Russell; Chapman, Clark; Durda, Dan; Hut, Piet

    2006-01-01

    The Asteroid Tugboat (AT) is a fully controlled asteroid deflection concept using a robotic spacecraft powered by a high efficiency, electric propulsion system (ion or plasma) which docks with and attaches to the asteroid, conducts preliminary operations, and then thrusts continuously parallel to the asteroid velocity vector until the desired velocity change is achieved. Based on early warning, provided by ground tracking and orbit prediction, it would be deployed a decade or more prior to a ...

  17. Geography of the asteroid belt

    Science.gov (United States)

    Zellner, B. H.

    1978-01-01

    The CSM classification serves as the starting point on the geography of the asteroid belt. Raw data on asteroid types are corrected for observational biases (against dark objects, for instance) to derive the distribution of types throughout the belt. Recent work on family members indicates that dynamical families have a true physical relationship, presumably indicating common origin in the breakup of a parent asteroid.

  18. Rising Above the Storm: DIG TEXAS

    Science.gov (United States)

    Ellins, K. K.; Miller, K. C.; Bednarz, S. W.; Mosher, S.

    2011-12-01

    For a decade Texas educators, scientists and citizens have shown a commitment to earth science education through planning at the national and state levels, involvement in earth science curriculum and teacher professional development projects, and the creation of a model senior level capstone Earth and Space Science course first offered in 2010 - 2011. The Texas state standards for Earth and Space Science demonstrate a shift to rigorous content, career relevant skills and use of 21st century technology. Earth and Space Science standards also align with the Earth Science, Climate and Ocean Literacy framework documents. In spite of a decade of progress K-12 earth science education in Texas is in crisis. Many school districts do not offer Earth and Space Science, or are using the course as a contingency for students who fail core science subjects. The State Board for Educator Certification eliminated Texas' secondary earth science teacher certification in 2009, following the adoption of the new Earth and Space Science standards. This makes teachers with a composite teacher certification (biology, physics and chemistry) eligible to teach Earth and Space Science, as well other earth science courses (e.g., Aquatic Science, Environmental Systems/Science) even if they lack earth science content knowledge. Teaching materials recently adopted by the State Board of Education do not include Earth and Space Science resources. In July 2011 following significant budget cuts at the 20 Education Service Centers across Texas, the Texas Education Agency eliminated key staff positions in its curriculum division, including science. This "perfect storm" has created a unique opportunity for a university-based approach to confront the crisis in earth science education in Texas which the Diversity and Innovation in the Geosciences (DIG) TEXAS alliance aims to fulfill. Led by the Texas A&M University College of Geosciences and The University of Texas Jackson School of Geosciences, with

  19. Asteroid science by Gaia

    Science.gov (United States)

    Muinonen, Karri; Cellino, Alberto; Dell Oro, Aldo; Tanga, Paolo; Delbo, Marco; Mignard, Francois; Thuillot, William; Berthier, Jerome; Carry, Benoit; Hestroffer, Daniel; Granvik, Mikael; Fedorets, Grigori

    2016-07-01

    Since the start of its regular observing program in summer 2014, the Gaia mission has carried out systematic photometric, spectrometric, and astrometric observations of asteroids. In total, the unique capabilities of Gaia allow for the collection of an extensive and homogeneous data set of some 350,000 asteroids down to the limiting magnitude of G = 20.7 mag. The Gaia performance remains excellent over the entire available brightness range. Starting from 2003, a working group of European asteroid scientists has explored the main capabilities of the mission, defining the expected scientific impact on Solar System science. These results have served as a basis for developing the Gaia data reduction pipeline, within the framework of the Data Processing and Analysis Consortium (DPAC). We describe the distribution of the existing and forecoming Gaia observations in space and time for different categories of objects. We illustrate the peculiar properties of each single observation, as these properties will affect the subsequent exploitation of the mission data. We will review the expected performances of Gaia, basically as a function of magnitude and proper motion of the sources. We will further focus on the areas that will benefit from complementary observational campaigns to improve the scientific return of the mission, and on the involvement of the planetary science community as a whole in the exploitation of the Gaia survey. We will thus describe the current and future opportunities for ground-based observers and forthcoming changes brought by Gaia in some observational approaches, such as stellar occultations by transneptunian objects and asteroids. We will show first results from the daily, short-term processing of Gaia data, all the way from the onboard data acquisition to the ground-based processing. We illustrate the tools developed to compute predictions of asteroid observations, we discuss the procedures implemented by the daily processing, and we illustrate

  20. Threat Mitigation: The Asteroid Tugboat

    CERN Document Server

    Schweickart, R; Durda, D; Hut, P; Chapman, Clark; Durda, Dan; Hut, Piet; Schweickart, Russell

    2006-01-01

    The Asteroid Tugboat (AT) is a fully controlled asteroid deflection concept using a robotic spacecraft powered by a high efficiency, electric propulsion system (ion or plasma) which docks with and attaches to the asteroid, conducts preliminary operations, and then thrusts continuously parallel to the asteroid velocity vector until the desired velocity change is achieved. Based on early warning, provided by ground tracking and orbit prediction, it would be deployed a decade or more prior to a potential impact. On completion of the initial rendezvous with the near-Earth object (NEO) the AT would first reduce the uncertainty in the orbit of the asteroid via Earth tracking of its radio transponder while it is station keeping with the asteroid. If on analysis of tracking data a deflection is required the AT would execute a reconnaissance phase collecting and processing information about the physical characteristics of the asteroid to support subsequent operations. The AT would then dock at the appropriate pole (i....

  1. Asteroids, meteorites, and comets

    CERN Document Server

    Elkins-Tanton, Linda T

    2010-01-01

    Asteroids, Comets, and Meteorites provides students, researchers, and general readers with the most up-to-date information on this fascinating field. From the days of the dinosaurs to our modern environment, this book explores all aspects of these cosmic invaders.

  2. Asteroid Lightcurve Photometry

    Science.gov (United States)

    Harris, A. W.

    2004-05-01

    With the advent of modestly priced CCD cameras and computer controller and reduction software, amateurs can now do photometry on fainter targets than was possible even from large observatories only a decade or so ago. This has led to an explosion of lightcurve data that in turn has yielded rich results. We now have rotation periods for more than 1500 asteroids, extending down to objects only tens of meters in diameter, and well determined shapes and pole orientations of more than 100 objects. Among smaller asteroids, the dispersion in rotation rates ranges from minutes to months, with the slower ones mostly "tumbling," or in states of non-principal axis rotation. The fastest ones must be monolithic, as centrifugal force exceeds their gravity. But among those larger than a few hundred meters diameter, there is a "rotation barrier" at the rate where gravity and centrifugal force match, suggesting that most asteroids this large or larger are "rubble piles." The broad dispersion in spin rates, almost a bimodal distribution, has long been a mystery, but now appears likely to be due to thermal radiation torques from the randomly asymmetric shapes of small asteroids. This is a major paradigm shift from the past, where mutual collisions were considered to be the dominant (or only) evolutionary process affecting spins. Amateur observations have already contributed a great deal leading to this new view, and much remains to be done, providing abundant opportunities for amateur-professional collaborations.

  3. Digging Deeper: Looking Beyond Behavior to Discover Meaning

    Medline Plus

    Full Text Available ... Behavior to Discover Meaning A Unit of Four Online Lessons Digging Deeper: Looking Beyond Behavior to Discover ... Behavior to Discover Meaning. A Unit of Four Online Lessons. HHS/ACF/OHS/EHSNRC. 2006. English. Last ...

  4. Digging Deeper: Looking Beyond Behavior to Discover Meaning

    Medline Plus

    Full Text Available ... Email Client Print Español Digging Deeper: Looking Beyond Behavior to Discover Meaning A Unit of Four Online ... started ZIP Code Search Department of Health and Human Services Administration for Children and Families Office of ...

  5. Impact-Actuated Digging Tool for Lunar Excavation Project

    Data.gov (United States)

    National Aeronautics and Space Administration — Honeybee Robotics proposes to develop a vacuum compatible, impact-actuated digging tool for the excavation of frozen and compacted regolith on the lunar surface and...

  6. Multiple origins of asteroid pairs

    Science.gov (United States)

    Jacobson, Seth A.

    2016-01-01

    Rotationally fissioned asteroids produce unbound asteroid pairs that have very similar heliocentric orbits. Backward integration of their current heliocentric orbits provides an age of closest proximity that can be used to date the rotational fission event. Most asteroid pairs follow a predicted theoretical relationship between the primary spin period and the mass ratio of the two pair members that is a direct consequence of the YORP-induced rotational fission hypothesis. If the progenitor asteroid has strength, asteroid pairs may have higher mass ratios or faster rotating primaries. However, the process of secondary fission leaves the originally predicted trend unaltered. We also describe the characteristics of pair members produced by four alternative routes from a rotational fission event to an asteroid pair. Unlike direct formation from the event itself, the age of closest proximity of these pairs cannot generally be used to date the rotational fission event since considerable time may have passed.

  7. Multiple origins of asteroid pairs

    CERN Document Server

    Jacobson, Seth A

    2015-01-01

    Rotationally fissioned asteroids produce unbound daughter asteroids that have very similar heliocentric orbits. Backward integration of their current heliocentric orbits provides an age of closest proximity that can be used to date the rotational fission event. Most asteroid pairs follow a predicted theoretical relationship between the primary spin period and the mass ratio of the two pair members that is a direct consequence of the YORP-induced rotational fission hypothesis. If the progenitor asteroid has strength, asteroid pairs may have high mass ratios with possibly fast rotating primaries. However, secondary fission leaves the originally predicted trend unaltered. We also describe the characteristics of pair members produced by four alternative routes from a rotational fission event to an asteroid pair. Unlike direct formation from the event itself, the age of closest proximity of these pairs cannot generally be used to date the rotational fission event since considerable time may have passed.

  8. Asteroid Impact Monitoring

    Science.gov (United States)

    Milani, A.

    2006-06-01

    Some asteroids and comets with Earth-crossing orbit may impact our planet, thus we need to be able to identify the cases which could have a dangerous close approach within a century. This must be done as soon as such an asteroid is discovered, allowing for follow up observations which might contradict the impact possibility, and in the worst case to organize mitigation, possibly including deflection. The mathematical problem of predicting possible impacts, even with very low probabilities, has been solved by our group in the last few years. This paper presents the basic theory of these impact prediction, and discusses how they are practically used in the impact monitoring systems now operational, in particular the CLOMON2 robot of the Universities of Pisa and Valladolid.

  9. Asteroid family ages

    CERN Document Server

    Spoto, Federica; Knezevic, Zoran

    2015-01-01

    A new family classification, based on a catalog of proper elements with $\\sim 384,000$ numbered asteroids and on new methods is available. For the $45$ dynamical families with $>250$ members identified in this classification, we present an attempt to obtain statistically significant ages: we succeeded in computing ages for $37$ collisional families. We used a rigorous method, including a least squares fit of the two sides of a V-shape plot in the proper semimajor axis, inverse diameter plane to determine the corresponding slopes, an advanced error model for the uncertainties of asteroid diameters, an iterative outlier rejection scheme and quality control. The best available Yarkovsky measurement was used to estimate a calibration of the Yarkovsky effect for each family. The results are presented separately for the families originated in fragmentation or cratering events, for the young, compact families and for the truncated, one-sided families. For all the computed ages the corresponding uncertainties are pro...

  10. Asteroid Surface Geophysics

    CERN Document Server

    Murdoch, Naomi; Schwartz, Stephen R; Miyamoto, Hideaki

    2015-01-01

    The regolith-covered surfaces of asteroids preserve records of geophysical processes that have occurred both at their surfaces and sometimes also in their interiors. As a result of the unique micro-gravity environment that these bodies posses, a complex and varied geophysics has given birth to fascinating features that we are just now beginning to understand. The processes that formed such features were first hypothesised through detailed spacecraft observations and have been further studied using theoretical, numerical and experimental methods that often combine several scientific disciplines. These multiple approaches are now merging towards a further understanding of the geophysical states of the surfaces of asteroids. In this chapter we provide a concise summary of what the scientific community has learned so far about the surfaces of these small planetary bodies and the processes that have shaped them. We also discuss the state of the art in terms of experimental techniques and numerical simulations that...

  11. Silicates in Alien Asteroids

    Science.gov (United States)

    2009-01-01

    This plot of data from NASA's Spitzer Space Telescopes shows that asteroid dust around a dead 'white dwarf' star contains silicates a common mineral on Earth. The data were taken primarily by Spitzer's infrared spectrograph, an instrument that breaks light apart into its basic constituents. The yellow dots show averaged data from the spectrograph, while the orange triangles show older data from Spitzer's infrared array camera. The white dwarf is called GD 40.

  12. Comet or Asteroid?

    Science.gov (United States)

    1997-11-01

    When is a minor object in the solar system a comet? And when is it an asteroid? Until recently, there was little doubt. Any object that was found to display a tail or appeared diffuse was a comet of ice and dust grains, and any that didn't, was an asteroid of solid rock. Moreover, comets normally move in rather elongated orbits, while most asteroids follow near-circular orbits close to the main plane of the solar system in which the major planets move. However, astronomers have recently discovered some `intermediate' objects which seem to possess properties that are typical for both categories. For instance, a strange object (P/1996 N2 - Elst-Pizarro) was found last year at ESO ( ESO Press Photo 36/96 ) which showed a cometary tail, while moving in a typical asteroidal orbit. At about the same time, American scientists found another (1996 PW) that moved in a very elongated comet-type orbit but was completely devoid of a tail. Now, a group of European scientists, by means of observations carried out at the ESO La Silla observatory, have found yet another object that at first appeared to be one more comet/asteroid example. However, continued and more detailed observations aimed at revealing its true nature have shown that it is most probably a comet . Consequently, it has received the provisional cometary designation P/1997 T3 . The Uppsala-DLR Trojan Survey Some time ago, Claes-Ingvar Lagerkvist (Astronomical Observatory, Uppsala, Sweden), in collaboration with Gerhard Hahn, Stefano Mottola, Magnus Lundström and Uri Carsenty (DLR, Institute of Planetary Exploration, Berlin, Germany), started to study the distribution of asteroids near Jupiter. They were particularly interested in those that move in orbits similar to that of Jupiter and which are located `ahead' of Jupiter in the so-called `Jovian L4 Lagrangian point'. Together with those `behind' Jupiter, these asteroids have been given the names of Greek and Trojan Heroes who participated in the famous Trojan war

  13. Dig Hazard Assessment Using a Stereo Pair of Cameras

    Science.gov (United States)

    Rankin, Arturo L.; Trebi-Ollennu, Ashitey

    2012-01-01

    This software evaluates the terrain within reach of a lander s robotic arm for dig hazards using a stereo pair of cameras that are part of the lander s sensor system. A relative level of risk is calculated for a set of dig sectors. There are two versions of this software; one is designed to run onboard a lander as part of the flight software, and the other runs on a PC under Linux as a ground tool that produces the same results generated on the lander, given stereo images acquired by the lander and downlinked to Earth. Onboard dig hazard assessment is accomplished by executing a workspace panorama command sequence. This sequence acquires a set of stereo pairs of images of the terrain the arm can reach, generates a set of candidate dig sectors, and assesses the dig hazard of each candidate dig sector. The 3D perimeter points of candidate dig sectors are generated using configurable parameters. A 3D reconstruction of the terrain in front of the lander is generated using a set of stereo images acquired from the mast cameras. The 3D reconstruction is used to evaluate the dig goodness of each candidate dig sector based on a set of eight metrics. The eight metrics are: 1. The maximum change in elevation in each sector, 2. The elevation standard deviation in each sector, 3. The forward tilt of each sector with respect to the payload frame, 4. The side tilt of each sector with respect to the payload frame, 5. The maximum size of missing data regions in each sector, 6. The percentage of a sector that has missing data, 7. The roughness of each sector, and 8. Monochrome intensity standard deviation of each sector. Each of the eight metrics forms a goodness image layer where the goodness value of each sector ranges from 0 to 1. Goodness values of 0 and 1 correspond to high and low risk, respectively. For each dig sector, the eight goodness values are merged by selecting the lowest one. Including the merged goodness image layer, there are nine goodness image layers for each

  14. Evolutionary Pathways for Asteroid Satellites

    Science.gov (United States)

    Jacobson, Seth Andrew

    2015-08-01

    The YORP-induced rotational fission hypothesis is a proposed mechanism for the creation of small asteroid binaries, which make up approximately 1/6-th of the near-Earth asteroid and small Main Belt asteroid populations. The YORP effect is a radiative torque that rotationally accelerates asteroids on timescales of thousands to millions of years. As asteroids rotationally accelerate, centrifugal accelerations on material within the body can match gravitational accelerations holding that material in place. When this occurs, that material goes into orbit. Once in orbit that material coalesces into a companion that undergoes continued dynamical evolution.Observations with radar, photometric and direct imaging techniques reveal a diverse array of small asteroid satellites. These systems can be sorted into a number of morphologies according to size, multiplicity of members, dynamical orbit and spin states, and member shapes. For instance, singly synchronous binaries have short separation distances between the two members, rapidly rotating oblate primary members, and tidally locked prolate secondary members. Other confirmed binary morphologies include doubly synchronous, tight asynchronous and wide asynchronous binaries. Related to these binary morphologies are unbound paired asteroid systems and bi-lobate contact binaries.A critical test for the YORP-induced rotational fission hypothesis is whether the binary asteroids produced evolve to the observed binary and related systems. In this talk I will review how this evolution is believed to occur according to gravitational dynamics, mutual body tides and the binary YORP effect.

  15. Photometry of Karin family asteroids

    NARCIS (Netherlands)

    Hahn, G.; Mottola, S.; Sen, A. K.; Harris, A. W.; Kührt, E.; Mueller, M.

    2006-01-01

    We have performed photometric observations in the V-band of two asteroids belonging to the Karin asteroid family, (11728) Einer and (93690) 2000 VE21 , using the 2-m Himalayan Chandra Telescope, Hanle and 2k ×4k pixels CCD imager. We obtained measurements during two nights (November 25 and 26, 2005)

  16. New Paradigms For Asteroid Formation

    CERN Document Server

    Johansen, Anders; Cuzzi, Jeffrey N; Morbidelli, Alessandro; Gounelle, Matthieu

    2015-01-01

    Asteroids and meteorites provide key evidence on the formation of planetesimals in the Solar System. Asteroids are traditionally thought to form in a bottom-up process by coagulation within a population of initially km-scale planetesimals. However, new models challenge this idea by demonstrating that asteroids of sizes from 100 to 1000 km can form directly from the gravitational collapse of small particles which have organised themselves in dense filaments and clusters in the turbulent gas. Particles concentrate passively between eddies down to the smallest scales of the turbulent gas flow and inside large-scale pressure bumps and vortices. The streaming instability causes particles to take an active role in the concentration, by piling up in dense filaments whose friction on the gas reduces the radial drift compared to that of isolated particles. In this chapter we review new paradigms for asteroid formation and compare critically against the observed properties of asteroids as well as constraints from meteo...

  17. Radar Investigations of Asteroids

    Science.gov (United States)

    Ostro, S.

    2004-05-01

    Radar investigations have provided otherwise unavailable information about the physical and dynamical properties of about 230 asteroids. Measurements of the distribution of echo power in time delay (range) and Doppler frequency (line-of-sight velocity) provide two-dimensional images with spatial resolution as fine as a decameter. Sequences of delay-Doppler images can be used to produce geologically detailed three-dimensional models, to define the rotation state precisely, to constrain the internal density distribution, and to estimate the trajectory of the object's center of mass. Radar wavelengths (4 to 13 cm) and the observer's control of transmitted and received polarizations make the observations sensitive to near-surface bulk density and macroscopic structure. Since delay-Doppler measurements are orthogonal to optical angle measurements and typically have much finer fractional precision, they are powerful for refining orbits and prediction ephemerides. Such astrometric measurements can add decades or centuries to the interval over which an asteroid's close Earth approaches can accurately be predicted and can significantly refine collision probability estimates based on optical astrometry alone. In the highly unlikely case that a small body is on course for an Earth collision in this century, radar reconnaissance would almost immediately distinguish between an impact trajectory and a near miss and would dramatically reduce the difficulty and cost of any effort to prevent the collision. The sizes and rotation periods of radar-detected asteroids span more than four orders of magnitude. The observations have revealed both stony and metallic objects, elongated and nonconvex shapes as well as nearly featureless spheroids, small-scale morphology ranging from smoother than the lunar regolith to rougher than the rockiest terrain on Mars, craters and diverse linear structures, non-principal-axis spin states, contact binaries, and binary systems.

  18. Radar Observations of Asteroids

    Science.gov (United States)

    Ostro, S. J.

    2003-05-01

    During the past 25 years, radar investigations have provided otherwise unavailable information about the physical and dynamical properties of more than 200 asteroids. Measurements of the distribution of echo power in time delay and Doppler frequency provide two-dimensional images with spatial resolution as fine as a decameter. Sequences of delay-Doppler images can be used to produce geologically detailed three-dimensional models, to define the rotation state precisely, to constrain the internal density distribution, and to estimate the trajectory of the object's center of mass. Radar wavelengths (4 to 13 cm) and the observer's control of transmitted and received polarizations make the observations sensitive to near-surface bulk density and macroscopic structure. Since delay-Doppler positional measurements are orthogonal to optical angle measurements and typically have much finer fractional precision, they are powerful for refining orbits and prediction ephemerides. Radar astrometry can add decades or centuries to the interval over which an asteroid's close Earth approaches can accurately be predicted and can significantly refine collision probability estimates based on optical astrometry alone. In the highly unlikely case that a small body is on course for an Earth collision in this century, radar reconnaissance would almost immediately distinguish between an impact trajectory and a near miss and would dramatically reduce the difficulty and cost of any effort to prevent the collision. The sizes and rotation periods of radar-detected asteroids span more than four orders of magnitude. These observations have revealed both stony and metallic objects, elongated and nonconvex shapes as well as nearly featureless spheroids, small-scale morphology ranging from smoother than the lunar regolith to rougher than the rockiest terrain on Mars, craters and diverse linear structures, non-principal-axis spin states, contact binaries, and binary systems.

  19. Asteroids and Comets

    CERN Document Server

    Fernandez, Yanga R; Howell, Ellen S; Woodney, Laura M

    2015-01-01

    Asteroids and comets are remnants from the era of Solar System formation over 4.5 billion years ago, and therefore allow us to address two fundamental questions in astronomy: what was the nature of our protoplanetary disk, and how did the process of planetary accretion occur? The objects we see today have suffered many geophysically-relevant processes in the intervening eons that have altered their surfaces, interiors, and compositions. In this chapter we review our understanding of the origins and evolution of these bodies, discuss the wealth of science returned from spacecraft missions, and motivate important questions to be addressed in the future.

  20. File list: His.Dig.10.AllAg.Intestine,_Small [Chip-atlas[Archive

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  14. Ion Beam Shepherd for Asteroid Deflection

    CERN Document Server

    Bombardelli, C

    2011-01-01

    We present a novel concept to impart a continuous thrust to an Earth threatening asteroid from a hovering spacecraft without need for physical attachment nor gravitational interaction with the asteroid. The concept involves an ion thruster placed at a distance of a few asteroid diameters directing a stream of quasi-neutral plasma against the asteroid surface resulting into a net transferred momentum. As the transmitted force is independent of the asteroid mass and size the method allows deflecting subkilometer asteroids with a spacecraft much lighter when compared to a gravity tractor spacecraft of equal deflection capability. The finding could make low-cost asteroid deflection missions possible in the coming years.

  15. Small scale digital soil mapping in Southeastern Kenya

    NARCIS (Netherlands)

    Mora Vallejo, A.P.; Claessens, L.; Stoorvogel, J.J.; Heuvelink, G.B.M.

    2008-01-01

    Digital soil mapping techniques appear to be an interesting alternative for traditional soil survey techniques. However, most applications deal with (semi-)detailed soil surveys where soil variability is determined by a limited number of soil forming factors. The question that remains is whether dig

  16. Images of an Activated Asteroid

    Science.gov (United States)

    Kohler, Susanna

    2016-08-01

    In late April of this year, asteroid P/2016 G1 (PANSTARRS) was discovered streaking through space, a tail of dust extending behind it. What caused this asteroids dust activity?Asteroid or Comet?Images of asteroid P/2016 G1 at three different times: late April, late May, and mid June. The arrow in the center panel points out an asymmetric feature that can be explained if the asteroid initially ejected material in a single direction, perhaps due to an impact. [Moreno et al. 2016]Asteroid P/2016 G1 is an interesting case: though it has the orbital elements of a main-belt asteroid it orbits at just under three times the EarthSun distance, with an eccentricity of e ~ 0.21 its appearance is closer to that of a comet, with a dust tail extending 20 behind it.To better understand the nature and cause of this unusual asteroids activity, a team led by Fernando Moreno (Institute of Astrophysics of Andalusia, in Spain) performed deep observations of P/2016 G1 shortly after its discovery. The team used the 10.4-meter Great Canary Telescope to image the asteroid over the span of roughly a month and a half.A Closer Look at P/2016 G1P/2016 G1 lies in the inner region of the main asteroid belt, so it is unlikely to have any ices that suddenly sublimated, causing the outburst. Instead, Moreno and collaborators suggest that the asteroids tail may have been caused by an impact that disrupted the parent body.To test this idea, the team used computer simulations to model their observations of P/2016 G1s dust tail. Based on their models, they demonstrate that the asteroid was likely activated on February 10 2016 roughly 350 days before it reached perihelion in its orbit and its activity was a short-duration event, lasting only ~24 days. The teams models indicate that over these 24 days, the asteroid lost around 20 million kilograms of dust, and at its maximum activity level, it was ejecting around 8 kg/s!Comparison of the observation from late May (panel a) and two models: one in which

  17. Structural Stability of Asteroids

    Science.gov (United States)

    Hirabayashi, Toshi

    This thesis develops a technique for analyzing the internal structure of an irregularly shaped asteroid. This research focuses on asteroid (216) Kleopatra, a few-hundred-kilometer-sized main belt asteroid spinning about its maximum moment of inertia axis with a rotation period of 5.385 hours, to motivate the techniques. While Ostro et al. [117] reported its dog bone-like shape, estimation of its size has been actively discussed. There are at least three different size estimates: Ostro et al., Descamps et al., and Marchis et al. Descamps et al. reported that (216) Kleopatra has satellites and obtained the mass of this object. This research consists of determination of possible failure modes of (216) Kleopatra and its subsequent detailed stress analysis, with each part including an estimation of the internal structure. The first part of this thesis considers the failure mode of Kleopatra and evaluates the size from it. Possible failure modes are modeled as either material shedding from the surface or plastic failure of the internal structure. The surface shedding condition is met when a zero-velocity curve with the same energy level as one of the dynamical equilibrium points attaches to the surface at the slowest spin period, while the plastic failure condition is characterized by extending the theorem by Holsapple (2008) that the yield condition of the averaged stress over the whole volume is identical to an upper bound for global failure. The prime result shows that while surface shedding does not occur at the current spin period and thus cannot result in the formation of the satellites, the neck may be situated near its plastic deformation state. From the failure condition, we also find that the size estimated by Descamps et al. (2011) is the most structurally stable. The second part of this thesis discusses finite element analyses with an assumption of an elastic-perfectly plastic material and a non-associated flow rule. The yield condition is modeled as the

  18. Asteroid airburst altitude vs. strength

    Science.gov (United States)

    Robertson, Darrel; Wheeler, Lorien; Mathias, Donovan

    2016-10-01

    Small NEO asteroids (plans and emergency management.Strong asteroids, such as a monolithic boulder, fail and create peak energy deposition close to the altitude at which ram dynamic pressure exceeds the material cohesive strength. Weaker asteroids, such as a rubble pile, structurally fail at higher altitude, but it requires the increased aerodynamic pressure at lower altitude to disrupt and disperse the rubble. Consequently the resulting airbursts have a peak energy deposition at similar altitudes.In this study hydrocode simulations of the entry and break-up of small asteroids were performed to examine the effect of strength, size, composition, entry angle, and speed on the resulting airburst. This presentation will show movies of the simulations, the results of peak burst height, and the comparison to semi-analytical models.

  19. Asteroid named after CAS scientist

    Institute of Scientific and Technical Information of China (English)

    2007-01-01

    @@ An asteroid has been named after CAS astronomy historian XI Zezong with the approval of the International Minor Planet Nomenclature Committee (IMPNC), announced China's National Astronomical Observatories at CAS (NAOC) on 17 August.

  20. Solar wind tans young asteroids

    Science.gov (United States)

    2009-04-01

    A new study published in Nature this week reveals that asteroid surfaces age and redden much faster than previously thought -- in less than a million years, the blink of an eye for an asteroid. This study has finally confirmed that the solar wind is the most likely cause of very rapid space weathering in asteroids. This fundamental result will help astronomers relate the appearance of an asteroid to its actual history and identify any after effects of a catastrophic impact with another asteroid. ESO PR Photo 16a/09 Young Asteroids Look Old "Asteroids seem to get a ‘sun tan' very quickly," says lead author Pierre Vernazza. "But not, as for people, from an overdose of the Sun's ultraviolet radiation, but from the effects of its powerful wind." It has long been known that asteroid surfaces alter in appearance with time -- the observed asteroids are much redder than the interior of meteorites found on Earth [1] -- but the actual processes of this "space weathering" and the timescales involved were controversial. Thanks to observations of different families of asteroids [2] using ESO's New Technology Telescope at La Silla and the Very Large Telescope at Paranal, as well as telescopes in Spain and Hawaii, Vernazza's team have now solved the puzzle. When two asteroids collide, they create a family of fragments with "fresh" surfaces. The astronomers found that these newly exposed surfaces are quickly altered and change colour in less than a million years -- a very short time compared to the age of the Solar System. "The charged, fast moving particles in the solar wind damage the asteroid's surface at an amazing rate [3]", says Vernazza. Unlike human skin, which is damaged and aged by repeated overexposure to sunlight, it is, perhaps rather surprisingly, the first moments of exposure (on the timescale considered) -- the first million years -- that causes most of the aging in asteroids. By studying different families of asteroids, the team has also shown that an asteroid

  1. Near Earth Asteroid Scout Project

    Data.gov (United States)

    National Aeronautics and Space Administration — In considering targets for human asteroid missions, there are several major factors that will make a significant difference in assessment of mission risks that...

  2. Earthtech, Dig-Texas and Upward Bound: Outreach to At-Risk Students with Interdisciplinary STEM Activities

    Science.gov (United States)

    Olgin, J. G.; Güereque, M.; Pennington, D. D.; Everett, A.; Dixon, J. G.; Reyes, A.; Houser, P. I. Q.; Baker, J. A.; Stocks, E.; Ellins, K.

    2015-12-01

    The Geological Sciences department at the University of Texas at El Paso (UTEP) hosted the EarthTech outreach program - a one-week intensive summer camp for low-income, at-risk high school students. The EarthTech program engaged students in STEM activities from geological and environmental sciences. Developed and led by university student-mentors with guidance from a supervising faculty member, the course engaged Upward Bound students with lectures, interactive projects, and excursions to local ecological preserves and geological sites around El Paso, Texas. Topics covered plant and animal distribution and diversity, water and soil dynamics, evolution and paleontology, geohazards, and planetary science. Field trips were combined with hands-on activities, including activities from DIG Texas teaching modules. The NSF-funded DIG Texas Instructional Blueprints project is organizing vetted, high quality online educational resources and learning activities into teaching modules. The modules follow a storyline and demonstrate congruency with the Next Generation Science Standards. Selected DIG Texas resources were included in the daily curriculum to complement the field trip and other hands-on activities. EarthTech students created ESRI Online GIS story maps in which they showed the locations of the field trips, incorporated photographs they had taken, and provided written reflections about their camp experiences. The DIG Texas project evaluation collected survey and interview data from the university student mentors throughout the week to ascertain the efficacy of the program. This poster presentation will include an overview of the program, including examples of work and evaluation results.

  3. Scribing Work Songs at an Archeological Dig in Egypt

    Science.gov (United States)

    Poppe, Donna

    2011-01-01

    This article reports research conducted in the northeastern corner of Egypt's Nile Delta during an excavation at the Mendes archeological dig site in July-August, 2007. Donald Redford, Professor at Pennsylvania State University, accepted the author as the only nonarcheologist that year. In addition to duties of measuring, registering, and storing…

  4. Experimental analysis of the load on the bucket wheel by the digging process - Part 2

    Energy Technology Data Exchange (ETDEWEB)

    Hitzschke, K.; Jacob, K.

    1984-10-01

    Bench-scale experiments aimed at modeling the digging process of bucket wheel excavators are evaluated. The design of the laboratory bucket wheel digging machine as well as the arrangement of measuring devices are explained. Measurement values were computer processed with TAKRAF programs on model dynamics for heavy surface mining equipment. Various graphs show cutting force components for single digging teeth and for an asymmetrical digging vessel. Cutting is carried out in advancing and slewing direction. Functions for mean values of digging forces are given with which the load on the bucket wheel can be determined. The mathematical description of the digging process is a means of assessing geometrical design and digging performance of buckets.

  5. Rapid Divergence of Nesting Depth and Digging Appendages among Tunneling Dung Beetle Populations and Species.

    Science.gov (United States)

    Macagno, Anna L M; Moczek, Armin P; Pizzo, Astrid

    2016-05-01

    Many dung beetle communities are characterized by species that share very similar morphological, ecological, and behavioral traits and requirements yet appear to be stably maintained. Here, we document that the morphologically nearly indistinguishable, sympatric, and syntopic tunneling sister species Onthophagus taurus and Onthophagus illyricus may be avoiding competitive exclusion by nesting at remarkably different soil depths. Intriguingly, we also find rapid divergence in preferred nesting depth across native and recently established O. taurus populations. Furthermore, geometric morphometric analyses reveal that both inter- and intraspecific divergences in nesting depth are paralleled by similar changes in the shape of the primary digging appendages, the fore tibiae. Collectively, our results identify preferred nesting depth and tibial shape as surprisingly evolutionarily labile and with the potential to ease interspecific competition and/or to facilitate adaptation to local climatic conditions. PMID:27105002

  6. Asteroid Exploration and Exploitation

    Science.gov (United States)

    Lewis, John S.

    2006-01-01

    John S. Lewis is Professor of Planetary Sciences and Co-Director of the Space Engineering Research Center at the University of Arizona. He was previously a Professor of Planetary Sciences at MIT and Visiting Professor at the California Institute of Technology. Most recently, he was a Visiting Professor at Tsinghua University in Beijing for the 2005-2006 academic year. His research interests are related to the application of chemistry to astronomical problems, including the origin of the Solar System, the evolution of planetary atmospheres, the origin of organic matter in planetary environments, the chemical structure and history of icy satellites, the hazards of comet and asteroid bombardment of Earth, and the extraction, processing, and use of the energy and material resources of nearby space. He has served as member or Chairman of a wide variety of NASA and NAS advisory committees and review panels. He has written 17 books, including undergraduate and graduate level texts and popular science books, and has authored over 150 scientific publications.

  7. Asteroid secular dynamics: Ceres' fingerprint identified

    OpenAIRE

    Novaković, Bojan; Maurel, Clara; Tsirvoulis, Georgios; Knezević, Zoran

    2015-01-01

    Here we report on the significant role of a so far overlooked dynamical aspect, namely a secular resonance between the dwarf planet Ceres and other asteroids. We demonstrate that this type of secular resonance can be the dominant dynamical factor in certain regions of the main asteroid belt. Specifically, we performed a dynamical analysis of the asteroids belonging to the (1726) Hoffmeister family. To identify which dynamical mechanisms are actually at work in this part of the main asteroid b...

  8. Asteroid Systems: Binaries, Triples, and Pairs

    CERN Document Server

    Margot, Jean-Luc; Taylor, Patrick; Carry, Benoît; Jacobson, Seth

    2015-01-01

    In the past decade, the number of known binary near-Earth asteroids has more than quadrupled and the number of known large main belt asteroids with satellites has doubled. Half a dozen triple asteroids have been discovered, and the previously unrecognized populations of asteroid pairs and small main belt binaries have been identified. The current observational evidence confirms that small (20 km) binaries with small satellites are most likely created during large collisions.

  9. Reflectance spectroscopy and asteroid surface mineralogy

    Science.gov (United States)

    Gaffey, Michael J.; Bell, Jeffrey F.; Cruikshank, Dale P.

    1989-01-01

    Information available from reflectance spectroscopy on the surface mineralogy of asteroids is discussed. Current spectral interpretive procedures used in the investigations of asteroid mineralogy are described. Present understanding of the nature and history of asteroids is discussed together with some still unresolved issues such as the source of ordinary chondrites.

  10. A Gravitational Tractor for Towing Asteroids

    CERN Document Server

    Lu, E T; Lu, Edward T.; Categories, Stanley G. Love

    2005-01-01

    We present a concept for a spacecraft that can controllably alter the trajectory of an Earth threatening asteroid using gravity as a towline. The spacecraft hovers near the asteroid with thrusters angled outward so the exhaust does not impinge on the surface. This deflection method is insensitive to the structure, surface properties, and rotation state of the asteroid.

  11. Benchmarking Asteroid-Deflection Experiment

    Science.gov (United States)

    Remington, Tane; Bruck Syal, Megan; Owen, John Michael; Miller, Paul L.

    2016-10-01

    An asteroid impacting Earth could have devastating consequences. In preparation to deflect or disrupt one before it reaches Earth, it is imperative to have modeling capabilities that adequately simulate the deflection actions. Code validation is key to ensuring full confidence in simulation results used in an asteroid-mitigation plan. We are benchmarking well-known impact experiments using Spheral, an adaptive smoothed-particle hydrodynamics code, to validate our modeling of asteroid deflection. We describe our simulation results, compare them with experimental data, and discuss what we have learned from our work. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. LLNL-ABS-695540

  12. On the Astrid asteroid family

    CERN Document Server

    Carruba, V

    2016-01-01

    Among asteroid families, the Astrid family is peculiar because of its unusual inclination distribution. Objects at $a\\simeq$~2.764 au are quite dispersed in this orbital element, giving the family a "crab-like" appearance. Recent works showed that this feature is caused by the interaction of the family with the $s-s_C$ nodal secular resonance with Ceres, that spreads the inclination of asteroids near its separatrix. As a consequence, the currently observed distribution of the $v_W$ component of terminal ejection velocities obtained from inverting Gauss equation is quite leptokurtic, since this parameter mostly depends on the asteroids inclination. The peculiar orbital configuration of the Astrid family can be used to set constraints on key parameters describing the strength of the Yarkovsky force, such as the bulk and surface density and the thermal conductivity of surface material. By simulating various fictitious families with different values of these parameters, and by demanding that the current value of ...

  13. Reproductive ecology of Sichuan digging frogs (Microhylidae: Kaloula rugifera

    Directory of Open Access Journals (Sweden)

    Wei Chen

    2015-06-01

    Full Text Available Abstract. We investigated the reproductive ecology of Sichuan digging frogs (Microhylidae: Kaloula rugifera in Mianyang, China during the wet season of 2013. Male Sichuan digging frogs first appear at temporary ponds following the first heavy rain of the wet season and initiate calling. Females arrive at ponds shortly after males. Male frogs chorus extensively throughout the wet season during the evenings and nights following rainstorms. Female frogs leave the pond after laying eggs, and likely only lay one clutch annually. Amplexus lasted up to three hours. Females were larger than males in terms of body size, but we found no evidence of size-assortative mating. Clutch size varied from 920 to 2200 eggs, with egg diameter ranging from 1.33 to 1.93 mm. Larger female frogs laid more eggs, and there was no correlation between egg number and egg size. Tadpoles hatched from eggs within 18-20 hours of oviposition, and grew for 30-40 days before complete metamorphosis occurred. The initial body length of tadpoles ranged from 3-5 mm snout-vent length. Growth was fastest immediately after hatching, and declined asymptotically with increasing tadpole body size. Overall, Sichuan digging frogs have a breeding biology characterized by strong male-male competition with prolonged breeding coinciding with the annual wet season. Keywords. Breeding ecology; Kaloula rugifera; life history; mating system

  14. AsteroidZoo: A New Zooniverse project to detect asteroids and improve asteroid detection algorithms

    Science.gov (United States)

    Beasley, M.; Lewicki, C. A.; Smith, A.; Lintott, C.; Christensen, E.

    2013-12-01

    We present a new citizen science project: AsteroidZoo. A collaboration between Planetary Resources, Inc., the Zooniverse Team, and the Catalina Sky Survey, we will bring the science of asteroid identification to the citizen scientist. Volunteer astronomers have proved to be a critical asset in identification and characterization of asteroids, especially potentially hazardous objects. These contributions, to date, have required that the volunteer possess a moderate telescope and the ability and willingness to be responsive to observing requests. Our new project will use data collected by the Catalina Sky Survey (CSS), currently the most productive asteroid survey, to be used by anyone with sufficient interest and an internet connection. As previous work by the Zooniverse has demonstrated, the capability of the citizen scientist is superb at classification of objects. Even the best automated searches require human intervention to identify new objects. These searches are optimized to reduce false positive rates and to prevent a single operator from being overloaded with requests. With access to the large number of people in Zooniverse, we will be able to avoid that problem and instead work to produce a complete detection list. Each frame from CSS will be searched in detail, generating a large number of new detections. We will be able to evaluate the completeness of the CSS data set and potentially provide improvements to the automated pipeline. The data corpus produced by AsteroidZoo will be used as a training environment for machine learning challenges in the future. Our goals include a more complete asteroid detection algorithm and a minimum computation program that skims the cream of the data suitable for implemention on small spacecraft. Our goal is to have the site become live in the Fall 2013.

  15. Resonant Structure of the THEMIS Asteroid Family

    Science.gov (United States)

    Kehoe, T. J. J.; Murray, C. D.

    1996-09-01

    The existence of resonant structure associated with low-order Jovian mean-motion commensurabilities within the main asteroid belt is already well established. However, previous studies have also suggested evidence for gaps within individual asteroid families. Whereas the Kirkwood gaps in the main asteroid belt are known to result from the actual removal of asteroids from resonant locations, it is not clear if this is also the case for the gaps evident within asteroid families. Indeed, the fact that asteroid families are identified by clustering in proper element space prompted Dermott & Murray (1981) to suggest that some of these gaps might only result from a failure to identify asteroids undergoing resonant perturbations as family members. We have investigated this hypothesis for the particular case of the Themis family of asteroids by numerically integrating the orbits of a carefully created artificial asteroid family. The orbital elements for this artificial family were constructed with proper element distributions closely resembling those of the actual Themis family but with any resonant structure removed. These orbits were then evolved to determine whether asteroids were indeed being removed from resonant locations and to monitor the mechanisms by which this occurred. We present evidence which indicates that the 2:1 Jovian mean-motion resonance may have played an important role in depleting the original Themis asteroid family of some of its members.

  16. NASA's Asteroid Redirect Mission (ARM)

    Science.gov (United States)

    Abell, Paul; Mazanek, Dan; Reeves, David; Naasz, Bo; Cichy, Benjamin

    2015-11-01

    The National Aeronautics and Space Administration (NASA) is developing a robotic mission to visit a large near-Earth asteroid (NEA), collect a multi-ton boulder from its surface, and redirect it into a stable orbit around the Moon. Once returned to cislunar space in the mid-2020s, astronauts will explore the boulder and return to Earth with samples. This Asteroid Redirect Mission (ARM) is part of NASA’s plan to advance the technologies, capabilities, and spaceflight experience needed for a human mission to the Martian system in the 2030s. Subsequent human and robotic missions to the asteroidal material would also be facilitated by its return to cislunar space. Although ARM is primarily a capability demonstration mission (i.e., technologies and associated operations), there exist significant opportunities to advance our knowledge of small bodies in the synergistic areas of science, planetary defense, asteroidal resources and in-situ resource utilization (ISRU), and capability and technology demonstrations. In order to maximize the knowledge return from the mission, NASA is organizing an ARM Investigation Team, which is being preceded by the Formulation Assessment and Support Team. These teams will be comprised of scientists, technologists, and other qualified and interested individuals to help plan the implementation and execution of ARM. An overview of robotic and crewed segments of ARM, including the mission requirements, NEA targets, and mission operations, will be provided along with a discussion of the potential opportunities associated with the mission.

  17. Lightcurve Analysis of Fourteen Asteroids

    Science.gov (United States)

    Pray, Donald P.; Galad, Adrian; Husarik, Marek; Oey, Julian

    2008-03-01

    Lightcurve period and amplitude are reported for the following asteroids observed at Carbuncle Hill Observatory and other sites between December 2006 and March 2007: 1806 Derice, 2472 Bradman, 2480 Popanov, 2768 Gorky, 2874 Jim Young, 3314 Beals, 4936 Butakov, 5676 Voltaire, 6709 Hiromiyuki, 6737 Okabayashi, 9368 Eshashi, 13497 Ronstone, (14142) 1998 SG10 and (46598) 1993 FT2.

  18. Into the regolith: digging for hydrological tracers

    Science.gov (United States)

    Moragues-Quiroga, Cristina; Hissler, Christophe; Chabaux, François; Legout, Arnaud; Stille, Peter

    2016-04-01

    The mineralogical and trace element composition of regoliths is a source of potential tracers of water behaviour in catchment systems. We propose an assessment of the most suitable spatial tracers for water collection, mixing, storage and release processes by incorporating geochemical signatures derived from trace and major elements to the description of sources and pathways of water contributions in the stream. To date, stable isotopes are widely used to trace water sources and water transit times but they are still missing a complementary tool which allows for the identification of end-members and the understanding of mixing processes within the regolith. Trace elements are known to be powerful and precise geochemical tracers of environmental processes and, therefore, they can be useful indicators of the spatial origin and evolution of regolith materials and water chemistry. We studied a whole slate regolith profile for its mineralogical, major and trace element composition. The different regolith components were subjected to a leaching experiment in order to identify chemical zonations within and assess the potential elements mobility. Rain, soil, stream and ground waters were collected at the same location than the regolith system over 4 years, analysed for their trace and major elements composition and compared to regolith and regolith leachates data. The results deliver valuable information on exchange processes at the water-mineral interface in the different zones of the regolith. The geochemical scheme of a complete regolith and the waters it holds is here presented to prove the efficiency of trace and major elements as complementary hydrological and geochemical tracers of water migration throughout a regolith till the stream.

  19. The Asteroid Redirect Mission (ARM)

    Science.gov (United States)

    Abell, Paul; Gates, Michele; Johnson, Lindley; Chodas, Paul; Mazanek, Dan; Reeves, David; Ticker, Ronald

    2016-07-01

    To achieve its long-term goal of sending humans to Mars, the National Aeronautics and Space Administration (NASA) plans to proceed in a series of incrementally more complex human spaceflight missions. Today, human flight experience extends only to Low-Earth Orbit (LEO), and should problems arise during a mission, the crew can return to Earth in a matter of minutes to hours. The next logical step for human spaceflight is to gain flight experience in the vicinity of the Moon. These cis-lunar missions provide a "proving ground" for the testing of systems and operations while still accommodating an emergency return path to the Earth that would last only several days. Cis-lunar mission experience will be essential for more ambitious human missions beyond the Earth-Moon system, which will require weeks, months, or even years of transit time. In addition, NASA has been given a Grand Challenge to find all asteroid threats to human populations and know what to do about them. Obtaining knowledge of asteroid physical properties combined with performing technology demonstrations for planetary defense provide much needed information to address the issue of future asteroid impacts on Earth. Hence the combined objectives of human exploration and planetary defense give a rationale for the Asteroid Re-direct Mission (ARM). Mission Description: NASA's ARM consists of two mission segments: 1) the Asteroid Redirect Robotic Mission (ARRM), the first robotic mission to visit a large (greater than ~100 m diameter) near-Earth asteroid (NEA), collect a multi-ton boulder from its surface along with regolith samples, demonstrate a planetary defense technique, and return the asteroidal material to a stable orbit around the Moon; and 2) the Asteroid Redirect Crewed Mission (ARCM), in which astronauts will take the Orion capsule to rendezvous and dock with the robotic vehicle, conduct multiple extravehicular activities to explore the boulder, and return to Earth with samples. NASA's proposed

  20. BPA电网模型自动导入DIgSILENT的研究和开发%Research and development of BPA grid model imported to DIgSILENT

    Institute of Scientific and Technical Information of China (English)

    刘庆; 张东英; 刘燕华; 许晓艳; 黄越辉

    2014-01-01

    为了实现将BPA的电网模型自动导入到DIgSILENT/PowerFactory中,提高在DIgSILENT中进行大电网建模的工作效率,分析了 BPA 和 DIgSILENT 中一次设备的数学模型,给出了这两种仿真软件在一次设备模型参数间的转换公式。研究了DIgSILENT提供的DGS接口和DPL编程语言的功能和技术特点,总结了BPA电网模型导入DIgSILENT的工作步骤。研究确定了VC6和DPL相结合的技术实现方案,设计了用于将BPA电网模型自动导入到DIgSILENT的工具软件的总体结构、功能和流程,开发实现了该工具软件。最后分别用3机9节点算例和北京电网等值系统对其测试,通过对比两个仿真软件的一次设备模型参数和潮流计算结果,验证该工具软件达到了设计的要求。%To-automatically-import-the-BPA-grid-model-to-DIgSILENT/PowerFactory-and-improve-the-efficiency-of-large-power-grid-modeling-in-DIgSILENT,-this-paper-analyzes-the-mathematical-model-of-the-primary-equipment-and-gives-the-conversion-formula-of-model-parameters-between-these-two-simulation-software,-studies-the-functions-and-technical-characteristics-of-DGS-interface-and-DPL-programming-language-provided-by-DIgSILENT,-summarizes-the-work-steps-for-the-BPA-grid-model-imported-to-DIgSILENT,-identifies-the-VC6-and-DPL-combining-technical-implementation-and-designs-the-overall-structure,-function-and-process-of-the-tool-software-which-is-used-to-import-BPA-grid-model-to-DIgSILENT,-then-develops-this-tool-software.-At-last,-this-paper-uses-3-machine-9-bus-system-and-the-equivalent-system-of-the-Beijing-grid-to-test-the-tool-software.-By-comparing-the-model-parameters-and-power-flow-calculation-results-of-the-primary-equipment-in-BPA-and-DIgSILENT,-this-tool-software-is-proved-to-meet-the-design-requirement.

  1. Radish Harvester Design and Finite Element Analysis of Digging Shovel%白萝卜收获机挖掘铲参数的设计

    Institute of Scientific and Technical Information of China (English)

    周国龙; 张晋国; 王洪伟; 顾旭彪; 杨进; 刘利坤

    2016-01-01

    In this paper,radish China reaped by low efficiency and high cost problem, design a special green radish dig-ging shovel.First step by digging shovel destroy the radish and the contact force of the soil, radish, separating from the soil, the second step by artificial collecting bag and then finish the whole course of radish harvest.By establishing a geo-metric model of the digging shovel capacity determines the angle of alpha,the shovel length L and width of the shovel a and the back face height h.Suspension traction after the mining device adopts the way of mining radish, make green rad-ish harvest efficiency is greatly raised, device has the advantages of simple structure, low cost, has the extremely broad market application scenario.%针对我国白萝卜人工收获效率低、成本高等问题,设计出专用的白萝卜挖掘铲。工作时,第1步通过挖掘铲破坏白萝卜与土壤的接触力,使白萝卜与土壤分离,第2步由人工捡拾装袋进而完成白萝卜收获的全过程。通过建立挖掘铲的几何模型确定了入土角α、铲面长度L、铲面宽度 A和后端面高度 h。该挖掘装置采用后悬挂牵引的方式挖掘白萝卜,使白萝卜的收获效率大大提高,装置结构简易、成本低,具有极其广阔的市场应用场景。

  2. Asteroids. Prospective energy and material resources

    Energy Technology Data Exchange (ETDEWEB)

    Badescu, Viorel (ed.) [Bucharest Polytechnic Univ. (Romania). Candida Oancea Institute

    2013-11-01

    Recent research on Prospective Energy and Material Resources on Asteroids. Carefully edited book dedicated to Asteroids prospective energy and material resources. Written by leading experts in the field. The Earth has limited material and energy resources while these resources in space are virtually unlimited. Further development of humanity will require going beyond our planet and exploring of extraterrestrial resources and sources of unlimited power. Thus far, all missions to asteroids have been motivated by scientific exploration. However, given recent advancements in various space technologies, mining asteroids for resources is becoming ever more feasible. A significant portion of asteroids value is derived from their location; the required resources do not need to be lifted at a great expense from the surface of the Earth. Resources derived from Asteroid not only can be brought back to Earth but could also be used to sustain human exploration of space and permanent settlements in space. This book investigates asteroids' prospective energy and material resources. It is a collection of topics related to asteroid exploration, and utilization. It presents past and future technologies and solutions to old problems that could become reality in our life time. The book therefore is a great source of condensed information for specialists involved in current and impending asteroid-related activities and a good starting point for space researchers, inventors, technologists and potential investors. Written for researchers, engineers, and businessmen interested in asteroids' exploration and exploitation.

  3. Near Earth Asteroid Characteristics for Asteroid Threat Assessment

    Science.gov (United States)

    Dotson, J.; Wooden, D. H.; Bryson, K.; Ostrowski, D. R.

    2015-12-01

    Information about the physical characteristics of Near Earth Asteroids (NEAs) is needed to model behavior during atmospheric entry, to assess the risk of an impact, and to model possible mitigation techniques. The intrinsic properties of interest to entry and mitigation modelers, however, rarely are directly measureable. Instead we measure other properties and infer the intrinsic physical properties, so determining the complete set of characteristics of interest is far from straightforward. In addition, for the majority of NEAs, only the basic measurements exist so often properties must be inferred from statistics of the population of more completely characterized objects. We will provide an assessment of the current state of knowledge about the physical characteristics of importance to asteroid threat assessment. In addition, an ongoing effort to collate NEA characteristics into a readily accessible database for use by the planetary defense community will be discussed.

  4. Designing Asteroid Impact Scenario Trajectories

    Science.gov (United States)

    Chodas, Paul

    2016-05-01

    In order to study some of the technical and geopolitical issues of dealing with an asteroid on impact trajectory, a number of hypothetical impact scenarios have been presented over the last ten years or so. These have been used, for example, at several of the Planetary Defense Conferences (PDCs), as well as in tabletop exercises with the Federal Emergency Management Agency (FEMA), along with other government agencies. The exercise at the 2015 PDC involved most of the attendees, consisted of seven distinct steps (“injects”), and with all the presentations and discussions, took up nearly 10 hours of conference time. The trajectory for the PDC15 scenario was entirely realistic, and was posted ahead of the meeting. It was made available in the NEO Program’s Horizons ephemeris service so that users could , for example, design their own deflection missions. The simulated asteroid and trajectory had to meet numerous very exacting requirements: becoming observable on the very first day of the conference, yet remaining very difficult to observe for the following 7 years, and far enough away from Earth that it was out of reach of radar until just before impact. It had to be undetectable in the past, and yet provide multiple perihelion opportunities for deflection in the future. It had to impact in a very specific region of the Earth, a specific number of years after discovery. When observations of the asteroid are simulated to generate an uncertainty region, that entire region must impact the Earth along an axis that cuts across specific regions of the Earth, the “risk corridor”. This is important because asteroid deflections generally move an asteroid impact point along this corridor. One scenario had a requirement that the asteroid pass through a keyhole several years before impact. The PDC15 scenario had an additional constraint that multiple simulated kinetic impactor missions altered the trajectory at a deflection point midway between discovery and impact

  5. Hvad der ikke slår dig ihjel

    OpenAIRE

    Nürnberg, Therese; Albek, Ida; Jaffke, Eva; Møller, Maria

    2013-01-01

    This paper investigates the genres employed in Louise Bokkenheuser’s Hvad der ikke slår dig ihjel: reportager fra København og Bagdad. To do this, the paper examines the work itself, by conduc-ting a genre analysis of the text. The focus of this study is to determine the significance of utilizing both fictional and nonfictional genres and writing styles in the telling of Louise Bokkenheuser’s story. The paper will clarify and define the genres applied in the text, using various literary theor...

  6. File list: Oth.Dig.10.AllAg.Intestinal_crypt [Chip-atlas[Archive

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  7. File list: DNS.Dig.20.AllAg.Intestinal_villus [Chip-atlas[Archive

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  8. File list: NoD.Dig.10.AllAg.Intestines [Chip-atlas[Archive

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  12. File list: Oth.Dig.50.AllAg.Intestines [Chip-atlas[Archive

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  5. File list: Pol.Dig.10.AllAg.Intestinal_villus [Chip-atlas[Archive

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  6. File list: Unc.Dig.05.AllAg.Intestines [Chip-atlas[Archive

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  8. File list: DNS.Dig.05.AllAg.Intestinal_crypt [Chip-atlas[Archive

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  9. File list: Oth.Dig.20.AllAg.Intestinal_villus [Chip-atlas[Archive

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  10. File list: Pol.Dig.10.AllAg.Intestinal_adenoma [Chip-atlas[Archive

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  13. File list: His.Dig.10.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

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  18. File list: Unc.Dig.05.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.05.AllAg.Intestinal_stem_cells mm9 Unclassified Digestive tract Intestinal stem... cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.05.AllAg.Intestinal_stem_cells.bed ...

  19. File list: DNS.Dig.20.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.20.AllAg.Intestinal_stem_cells mm9 DNase-seq Digestive tract Intestinal stem... cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.20.AllAg.Intestinal_stem_cells.bed ...

  20. File list: Unc.Dig.10.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.10.AllAg.Intestinal_stem_cells mm9 Unclassified Digestive tract Intestinal stem... cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.10.AllAg.Intestinal_stem_cells.bed ...

  1. File list: Pol.Dig.10.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.10.AllAg.Intestinal_stem_cells mm9 RNA polymerase Digestive tract Intestinal stem... cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.10.AllAg.Intestinal_stem_cells.bed ...

  2. File list: Pol.Dig.50.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.50.AllAg.Intestinal_stem_cells mm9 RNA polymerase Digestive tract Intestinal stem... cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.50.AllAg.Intestinal_stem_cells.bed ...

  3. File list: His.Dig.50.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.50.AllAg.Intestinal_stem_cells mm9 Histone Digestive tract Intestinal stem ...cells SRX856959,SRX193722 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/His.Dig.50.AllAg.Intestinal_stem_cells.bed ...

  4. File list: ALL.Dig.05.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Intestinal_stem_cells mm9 All antigens Digestive tract Intestinal stem...p://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.05.AllAg.Intestinal_stem_cells.bed ...

  5. File list: NoD.Dig.10.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.10.AllAg.Stomach hg19 No description Digestive tract Stomach SRX252720,SRX2...52731,SRX252741,SRX252737,SRX252723,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.10.AllAg.Stomach.bed ...

  6. File list: NoD.Dig.05.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.05.AllAg.Stomach hg19 No description Digestive tract Stomach SRX252720,SRX2...52731,SRX252741,SRX252737,SRX252723,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.05.AllAg.Stomach.bed ...

  7. File list: ALL.Dig.50.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.Stomach hg19 All antigens Digestive tract Stomach SRX252741,SRX252...01194,SRX121286,SRX055202,SRX121291,SRX214043,SRX252723,SRX055185,SRX055192,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.50.AllAg.Stomach.bed ...

  8. File list: His.Dig.05.AllAg.Caco-2 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.05.AllAg.Caco-2 hg19 Histone Digestive tract Caco-2 SRX189989,SRX189945,SRX...189986 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.05.AllAg.Caco-2.bed ...

  9. File list: His.Dig.10.Pan_lysine_crotonylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.10.Pan_lysine_crotonylation.AllCell mm9 Histone Pan lysine crotonylation Di...gestive tract http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/His.Dig.10.Pan_lysine_crotonylation.AllCell.bed ...

  10. File list: His.Dig.20.Pan_lysine_crotonylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.20.Pan_lysine_crotonylation.AllCell mm9 Histone Pan lysine crotonylation Di...gestive tract http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/His.Dig.20.Pan_lysine_crotonylation.AllCell.bed ...

  11. File list: His.Dig.05.Pan_lysine_crotonylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.05.Pan_lysine_crotonylation.AllCell hg19 Histone Pan lysine crotonylation D...igestive tract http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.05.Pan_lysine_crotonylation.AllCell.bed ...

  12. File list: Oth.Dig.05.Crotonyl_lysine.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.Crotonyl_lysine.AllCell mm9 TFs and others Crotonyl lysine Digestive tra...ct http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.05.Crotonyl_lysine.AllCell.bed ...

  13. File list: Oth.Dig.50.Crotonyl_lysine.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.50.Crotonyl_lysine.AllCell mm9 TFs and others Crotonyl lysine Digestive tra...ct http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.50.Crotonyl_lysine.AllCell.bed ...

  14. File list: NoD.Dig.50.AllAg.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.50.AllAg.AllCell hg19 No description Digestive tract SRX335279,SRX335159,SR...00,SRX335150 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.50.AllAg.AllCell.bed ...

  15. File list: Pol.Dig.50.AllAg.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.50.AllAg.AllCell hg19 RNA polymerase Digestive tract SRX100519,SRX295043,SR...078869,SRX1078862,SRX1078873,SRX1078877,SRX1078879,SRX1078878,SRX1078880 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.50.AllAg.AllCell.bed ...

  16. File list: InP.Dig.50.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.50.AllAg.Colon_cancer hg19 Input control Digestive tract Colon cancer SRX12...155774,SRX124693,SRX124698 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.50.AllAg.Colon_cancer.bed ...

  17. File list: InP.Dig.05.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.05.AllAg.Colon_cancer hg19 Input control Digestive tract Colon cancer SRX12...124693,SRX124695,SRX124694 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.05.AllAg.Colon_cancer.bed ...

  18. File list: Unc.Dig.10.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.10.AllAg.Colon_cancer hg19 Unclassified Digestive tract Colon cancer SRX115...0169,SRX124703,SRX1150170 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.10.AllAg.Colon_cancer.bed ...

  19. File list: Oth.Dig.50.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.50.AllAg.Colon_cancer hg19 TFs and others Digestive tract Colon cancer SRX1...55772,SRX155775,SRX155773,SRX155776 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.50.AllAg.Colon_cancer.bed ...

  20. File list: Oth.Dig.05.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Colon_cancer hg19 TFs and others Digestive tract Colon cancer SRX1...55772,SRX155773,SRX155775,SRX155776 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.AllAg.Colon_cancer.bed ...

  1. File list: Oth.Dig.10.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.AllAg.Colon_cancer hg19 TFs and others Digestive tract Colon cancer SRX1...55772,SRX155775,SRX155773,SRX155776 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.10.AllAg.Colon_cancer.bed ...

  2. File list: Unc.Dig.50.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.50.AllAg.Colon_cancer hg19 Unclassified Digestive tract Colon cancer SRX115...0169,SRX1150170,SRX124703 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.50.AllAg.Colon_cancer.bed ...

  3. File list: Oth.Dig.20.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.AllAg.Colon_cancer hg19 TFs and others Digestive tract Colon cancer SRX1...55772,SRX155773,SRX155775,SRX155776 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.20.AllAg.Colon_cancer.bed ...

  4. File list: InP.Dig.10.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.AllAg.Colon_cancer hg19 Input control Digestive tract Colon cancer SRX12...155774,SRX625671,SRX155777 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.10.AllAg.Colon_cancer.bed ...

  5. File list: Unc.Dig.05.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.05.AllAg.Colon_cancer hg19 Unclassified Digestive tract Colon cancer SRX115...0169,SRX1150170,SRX124703 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.05.AllAg.Colon_cancer.bed ...

  6. File list: InP.Dig.20.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.20.AllAg.Colon_cancer hg19 Input control Digestive tract Colon cancer SRX12...124693,SRX124697,SRX124698 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.20.AllAg.Colon_cancer.bed ...

  7. File list: Unc.Dig.20.AllAg.Colon_cancer [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.20.AllAg.Colon_cancer hg19 Unclassified Digestive tract Colon cancer SRX115...0169,SRX1150170,SRX124703 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.20.AllAg.Colon_cancer.bed ...

  8. File list: ALL.Dig.50.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.Gastric_tumor mm9 All antigens Digestive tract Gastric tumor SRX31...5102,SRX315096,SRX315100,SRX315094,SRX315095,SRX315101 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.50.AllAg.Gastric_tumor.bed ...

  9. File list: His.Dig.05.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.05.AllAg.Gastric_primary_sample hg19 Histone Digestive tract Gastric primar...105,SRX369094,SRX369095 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.05.AllAg.Gastric_primary_sample.bed ...

  10. File list: ALL.Dig.20.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.Gastric_tumor mm9 All antigens Digestive tract Gastric tumor SRX31...5102,SRX315096,SRX315100,SRX315094,SRX315095,SRX315101 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.20.AllAg.Gastric_tumor.bed ...

  11. File list: Pol.Dig.50.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.50.AllAg.Gastric_primary_sample hg19 RNA polymerase Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.50.AllAg.Gastric_primary_sample.bed ...

  12. File list: Pol.Dig.20.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.20.AllAg.Gastric_primary_sample hg19 RNA polymerase Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.20.AllAg.Gastric_primary_sample.bed ...

  13. File list: DNS.Dig.50.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.50.AllAg.Gastric_primary_sample hg19 DNase-seq Digestive tract Gastric prim...ary sample SRX201807,SRX201812 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.50.AllAg.Gastric_primary_sample.bed ...

  14. File list: Pol.Dig.05.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.05.AllAg.Gastric_primary_sample hg19 RNA polymerase Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.05.AllAg.Gastric_primary_sample.bed ...

  15. File list: Oth.Dig.50.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.50.AllAg.Gastric_primary_sample hg19 TFs and others Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.50.AllAg.Gastric_primary_sample.bed ...

  16. File list: Unc.Dig.05.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.05.AllAg.Gastric_primary_sample hg19 Unclassified Digestive tract Gastric p...rimary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.05.AllAg.Gastric_primary_sample.bed ...

  17. File list: Unc.Dig.50.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.50.AllAg.Gastric_primary_sample hg19 Unclassified Digestive tract Gastric p...rimary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.50.AllAg.Gastric_primary_sample.bed ...

  18. File list: Oth.Dig.05.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Gastric_primary_sample hg19 TFs and others Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.AllAg.Gastric_primary_sample.bed ...

  19. File list: DNS.Dig.05.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.05.AllAg.Gastric_primary_sample hg19 DNase-seq Digestive tract Gastric prim...ary sample SRX201807,SRX201812 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.05.AllAg.Gastric_primary_sample.bed ...

  20. File list: Oth.Dig.10.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.AllAg.Gastric_tumor mm9 TFs and others Digestive tract Gastric tumor SRX...315102,SRX315094,SRX315095,SRX315096,SRX315100,SRX315101 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.10.AllAg.Gastric_tumor.bed ...

  1. File list: DNS.Dig.20.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.20.AllAg.Gastric_primary_sample hg19 DNase-seq Digestive tract Gastric prim...ary sample SRX201807,SRX201812 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.20.AllAg.Gastric_primary_sample.bed ...

  2. File list: DNS.Dig.10.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.10.AllAg.Gastric_primary_sample hg19 DNase-seq Digestive tract Gastric prim...ary sample SRX201807,SRX201812 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.10.AllAg.Gastric_primary_sample.bed ...

  3. File list: Unc.Dig.20.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.20.AllAg.Gastric_primary_sample hg19 Unclassified Digestive tract Gastric p...rimary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Unc.Dig.20.AllAg.Gastric_primary_sample.bed ...

  4. File list: His.Dig.20.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.20.AllAg.Gastric_primary_sample hg19 Histone Digestive tract Gastric primar...096,SRX369094,SRX369095 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.20.AllAg.Gastric_primary_sample.bed ...

  5. File list: Oth.Dig.20.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.AllAg.Gastric_primary_sample hg19 TFs and others Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.20.AllAg.Gastric_primary_sample.bed ...

  6. File list: His.Dig.10.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.10.AllAg.Gastric_primary_sample hg19 Histone Digestive tract Gastric primar...095,SRX369094,SRX369099 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.10.AllAg.Gastric_primary_sample.bed ...

  7. File list: Oth.Dig.20.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.AllAg.Gastric_tumor mm9 TFs and others Digestive tract Gastric tumor SRX...315102,SRX315096,SRX315100,SRX315094,SRX315095,SRX315101 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.20.AllAg.Gastric_tumor.bed ...

  8. File list: ALL.Dig.10.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Gastric_tumor mm9 All antigens Digestive tract Gastric tumor SRX31...5102,SRX315094,SRX315095,SRX315096,SRX315100,SRX315101 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.10.AllAg.Gastric_tumor.bed ...

  9. File list: Oth.Dig.10.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.AllAg.Gastric_primary_sample hg19 TFs and others Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.10.AllAg.Gastric_primary_sample.bed ...

  10. File list: Oth.Dig.05.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Gastric_tumor mm9 TFs and others Digestive tract Gastric tumor SRX...315102,SRX315095,SRX315094,SRX315096,SRX315101,SRX315100 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.05.AllAg.Gastric_tumor.bed ...

  11. File list: ALL.Dig.05.AllAg.Gastric_tumor [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Gastric_tumor mm9 All antigens Digestive tract Gastric tumor SRX31...5102,SRX315095,SRX315094,SRX315096,SRX315101,SRX315100 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.05.AllAg.Gastric_tumor.bed ...

  12. File list: Pol.Dig.10.AllAg.Gastric_primary_sample [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.10.AllAg.Gastric_primary_sample hg19 RNA polymerase Digestive tract Gastric... primary sample http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.10.AllAg.Gastric_primary_sample.bed ...

  13. File list: His.Dig.50.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.50.AllAg.AGS hg19 Histone Digestive tract AGS SRX482979,SRX482980,SRX482982...,SRX482978,SRX482983,SRX482985,SRX482981,SRX482984 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.50.AllAg.AGS.bed ...

  14. File list: Oth.Dig.20.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.AllAg.AGS hg19 TFs and others Digestive tract AGS SRX367641,SRX371981,SR...X367642,SRX367640 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.20.AllAg.AGS.bed ...

  15. File list: Oth.Dig.10.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.AllAg.AGS hg19 TFs and others Digestive tract AGS SRX367641,SRX367642,SR...X371981,SRX367640 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.10.AllAg.AGS.bed ...

  16. File list: ALL.Dig.05.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.AGS hg19 All antigens Digestive tract AGS SRX367641,SRX367642,SRX3...X482983 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.05.AllAg.AGS.bed ...

  17. File list: His.Dig.05.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.05.AllAg.AGS hg19 Histone Digestive tract AGS SRX482980,SRX482979,SRX482981...,SRX482978,SRX482984,SRX482982,SRX482985,SRX482983 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.05.AllAg.AGS.bed ...

  18. File list: ALL.Dig.10.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.AGS hg19 All antigens Digestive tract AGS SRX367641,SRX367642,SRX3...X482983 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.10.AllAg.AGS.bed ...

  19. File list: His.Dig.20.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.20.AllAg.AGS hg19 Histone Digestive tract AGS SRX482980,SRX482979,SRX482981...,SRX482978,SRX482982,SRX482983,SRX482985,SRX482984 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.20.AllAg.AGS.bed ...

  20. File list: Oth.Dig.05.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.AGS hg19 TFs and others Digestive tract AGS SRX367641,SRX367642,SR...X371981,SRX367640 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.AllAg.AGS.bed ...

  1. File list: Oth.Dig.50.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.50.AllAg.AGS hg19 TFs and others Digestive tract AGS SRX367641,SRX371981,SR...X367642,SRX367640 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.50.AllAg.AGS.bed ...

  2. File list: ALL.Dig.50.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.AGS hg19 All antigens Digestive tract AGS SRX367641,SRX371982,SRX3...X367640 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.50.AllAg.AGS.bed ...

  3. File list: ALL.Dig.20.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.AGS hg19 All antigens Digestive tract AGS SRX367641,SRX371982,SRX3...X367640 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.20.AllAg.AGS.bed ...

  4. File list: His.Dig.10.AllAg.AGS [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.10.AllAg.AGS hg19 Histone Digestive tract AGS SRX482979,SRX482980,SRX482981...,SRX482984,SRX482978,SRX482982,SRX482985,SRX482983 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.10.AllAg.AGS.bed ...

  5. File list: DNS.Dig.05.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.05.AllAg.Stomach hg19 DNase-seq Digestive tract Stomach SRX089271,SRX100995...91,SRX055192,SRX214043 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.05.AllAg.Stomach.bed ...

  6. File list: ALL.Dig.20.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.Stomach hg19 All antigens Digestive tract Stomach SRX252741,SRX252...01194,SRX121286,SRX055202,SRX121291,SRX055185,SRX214043,SRX055192,SRX252723,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.20.AllAg.Stomach.bed ...

  7. File list: NoD.Dig.20.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.20.AllAg.Stomach hg19 No description Digestive tract Stomach SRX252741,SRX2...52720,SRX252731,SRX252737,SRX252723,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.20.AllAg.Stomach.bed ...

  8. File list: NoD.Dig.50.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.50.AllAg.Stomach hg19 No description Digestive tract Stomach SRX252741,SRX2...52720,SRX252731,SRX252737,SRX252723,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.50.AllAg.Stomach.bed ...

  9. File list: ALL.Dig.10.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Stomach hg19 All antigens Digestive tract Stomach SRX252720,SRX252...21286,SRX055202,SRX201194,SRX055185,SRX121291,SRX055192,SRX214043,SRX252723,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.10.AllAg.Stomach.bed ...

  10. File list: Oth.Dig.50.VSV-G.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.50.VSV-G.AllCell hg19 TFs and others VSV-G Digestive tract SRX961218,SRX961...219 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.50.VSV-G.AllCell.bed ...

  11. File list: Oth.Dig.20.VSV-G.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.VSV-G.AllCell hg19 TFs and others VSV-G Digestive tract SRX961218,SRX961...219 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.20.VSV-G.AllCell.bed ...

  12. File list: Oth.Dig.05.VSV-G.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.VSV-G.AllCell hg19 TFs and others VSV-G Digestive tract SRX961218,SRX961...219 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.VSV-G.AllCell.bed ...

  13. File list: Oth.Dig.10.VSV-G.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.VSV-G.AllCell hg19 TFs and others VSV-G Digestive tract SRX961218,SRX961...219 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.10.VSV-G.AllCell.bed ...

  14. File list: Pol.Dig.10.RNA_polymerase_II.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.10.RNA_polymerase_II.AllCell hg19 RNA polymerase RNA polymerase II Digestiv...//dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.10.RNA_polymerase_II.AllCell.bed ...

  15. File list: Oth.Dig.10.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.AllAg.Intestinal_stem_cells mm9 TFs and others Digestive tract Intestinal st...em cells SRX1141904,SRX856961,SRX1141903 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.10.AllAg.Intestinal_stem_cells.bed ...

  16. File list: DNS.Dig.50.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.50.AllAg.Intestinal_stem_cells mm9 DNase-seq Digestive tract Intestinal ste...m cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.50.AllAg.Intestinal_stem_cells.bed ...

  17. File list: Pol.Dig.05.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.05.AllAg.Intestinal_stem_cells mm9 RNA polymerase Digestive tract Intestinal st...em cells http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.05.AllAg.Intestinal_stem_cells.bed ...

  18. File list: Oth.Dig.10.Cdx2.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.Cdx2.AllCell mm9 TFs and others Cdx2 Digestive tract SRX028555,SRX112502...,SRX112503,SRX112504 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.10.Cdx2.AllCell.bed ...

  19. File list: NoD.Dig.20.AllAg.Esophagus [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.20.AllAg.Esophagus hg19 No description Digestive tract Esophagus SRX190764,...0 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.20.AllAg.Esophagus.bed ...

  20. File list: NoD.Dig.10.AllAg.Esophagus [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.10.AllAg.Esophagus hg19 No description Digestive tract Esophagus SRX136969,...0 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.10.AllAg.Esophagus.bed ...

  1. File list: NoD.Dig.50.AllAg.Esophagus [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.50.AllAg.Esophagus hg19 No description Digestive tract Esophagus SRX190764,...0 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.50.AllAg.Esophagus.bed ...

  2. File list: NoD.Dig.05.AllAg.Esophagus [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.05.AllAg.Esophagus hg19 No description Digestive tract Esophagus SRX134731,...5 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.05.AllAg.Esophagus.bed ...

  3. File list: ALL.Dig.10.AllAg.Intestine,_Small [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Intestine,_Small hg19 All antigens Digestive tract Intestine, Smal...7272,SRX142119,SRX157637,SRX263906,SRX136956,SRX213497 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.10.AllAg.Intestine,_Small.bed ...

  4. File list: NoD.Dig.10.AllAg.Intestine,_Small [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.10.AllAg.Intestine,_Small hg19 No description Digestive tract Intestine, Smal...90797,SRX263903,SRX263916,SRX347272,SRX142119,SRX157637,SRX263906,SRX136956,SRX213497 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/NoD.Dig.10.AllAg.Intestine,_Small.bed ...

  5. File list: His.Dig.50.Pan_lysine_crotonylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.50.Pan_lysine_crotonylation.AllCell hg19 Histone Pan lysine crotonylation D...igestive tract http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.50.Pan_lysine_crotonylation.AllCell.bed ...

  6. File list: Oth.Dig.05.AllAg.Crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Crypt mm9 TFs and others Digestive tract Crypt SRX365692,SRX856963...,SRX856958,SRX856962,SRX396312,SRX648716 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.05.AllAg.Crypt.bed ...

  7. File list: InP.Dig.05.AllAg.Crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.05.AllAg.Crypt hg19 Input control Digestive tract Crypt SRX124701,SRX124700...,SRX124702 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.05.AllAg.Crypt.bed ...

  8. File list: ALL.Dig.10.AllAg.Crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Crypt mm9 All antigens Digestive tract Crypt SRX365690,SRX365691,S...,SRX856956,SRX856957,SRX396312,SRX365694,SRX648716 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.10.AllAg.Crypt.bed ...

  9. File list: His.Dig.10.Pan_lysine_acetylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.10.Pan_lysine_acetylation.AllCell mm9 Histone Pan lysine acetylation Digest...ive tract http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/His.Dig.10.Pan_lysine_acetylation.AllCell.bed ...

  10. File list: His.Dig.20.Pan_lysine_acetylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.20.Pan_lysine_acetylation.AllCell hg19 Histone Pan lysine acetylation Diges...tive tract http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.20.Pan_lysine_acetylation.AllCell.bed ...

  11. File list: His.Dig.50.Pan_lysine_acetylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.50.Pan_lysine_acetylation.AllCell hg19 Histone Pan lysine acetylation Diges...tive tract http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.50.Pan_lysine_acetylation.AllCell.bed ...

  12. File list: His.Dig.05.Pan_lysine_acetylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.05.Pan_lysine_acetylation.AllCell mm9 Histone Pan lysine acetylation Digest...ive tract http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/His.Dig.05.Pan_lysine_acetylation.AllCell.bed ...

  13. File list: His.Dig.10.Pan_lysine_acetylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.10.Pan_lysine_acetylation.AllCell hg19 Histone Pan lysine acetylation Diges...tive tract http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.10.Pan_lysine_acetylation.AllCell.bed ...

  14. File list: His.Dig.05.Pan_lysine_acetylation.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.05.Pan_lysine_acetylation.AllCell hg19 Histone Pan lysine acetylation Diges...tive tract http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.05.Pan_lysine_acetylation.AllCell.bed ...

  15. File list: Oth.Dig.20.Vdr.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.Vdr.AllCell mm9 TFs and others Vdr Digestive tract SRX1037022,SRX1037021...,SRX1037020,SRX1037019,SRX1037018,SRX1037017 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.20.Vdr.AllCell.bed ...

  16. File list: Oth.Dig.05.Vdr.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.Vdr.AllCell mm9 TFs and others Vdr Digestive tract SRX1037022,SRX1037019...,SRX1037020,SRX1037021,SRX1037018,SRX1037017 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.05.Vdr.AllCell.bed ...

  17. File list: Oth.Dig.10.Vdr.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.Vdr.AllCell mm9 TFs and others Vdr Digestive tract SRX1037022,SRX1037021...,SRX1037020,SRX1037019,SRX1037018,SRX1037017 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.10.Vdr.AllCell.bed ...

  18. File list: ALL.Dig.50.AllAg.GIST-48 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.GIST-48 hg19 All antigens Digestive tract GIST-48 SRX825987,SRX023...216,SRX023215,SRX825986 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.50.AllAg.GIST-48.bed ...

  19. File list: ALL.Dig.20.AllAg.GIST-48 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.GIST-48 hg19 All antigens Digestive tract GIST-48 SRX825987,SRX023...216,SRX825986,SRX023215 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.20.AllAg.GIST-48.bed ...

  20. File list: ALL.Dig.10.AllAg.GIST-48 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.GIST-48 hg19 All antigens Digestive tract GIST-48 SRX825987,SRX023...216,SRX023215,SRX825986 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.10.AllAg.GIST-48.bed ...

  1. File list: InP.Dig.20.Input_control.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.20.Input_control.AllCell hg19 Input control Input control Digestive tract S...X077858,SRX286206,SRX124697,SRX1183967,SRX124698,SRX543691 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.20.Input_control.AllCell.bed ...

  2. File list: InP.Dig.50.Input_control.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.50.Input_control.AllCell hg19 Input control Input control Digestive tract S...RX155744,SRX612781,SRX543681,SRX101310,SRX648244,SRX863785 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.50.Input_control.AllCell.bed ...

  3. File list: InP.Dig.10.Input_control.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.Input_control.AllCell mm9 Input control Input control Digestive tract SR...X193725,ERX040284,SRX376981 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.10.Input_control.AllCell.bed ...

  4. File list: InP.Dig.05.Input_control.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.05.Input_control.AllCell hg19 Input control Input control Digestive tract S...RX124694,SRX543691,SRX543683,SRX367635,SRX286206,SRX543682 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.05.Input_control.AllCell.bed ...

  5. File list: InP.Dig.10.Input_control.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.Input_control.AllCell hg19 Input control Input control Digestive tract S...RX155777,SRX077858,SRX863785,SRX543682,SRX286206,SRX543691 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.10.Input_control.AllCell.bed ...

  6. File list: Pol.Dig.50.RNA_polymerase_II.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.50.RNA_polymerase_II.AllCell hg19 RNA polymerase RNA polymerase II Digestiv...//dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Pol.Dig.50.RNA_polymerase_II.AllCell.bed ...

  7. File list: Pol.Dig.05.RNA_Polymerase_II.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.05.RNA_Polymerase_II.AllCell mm9 RNA polymerase RNA Polymerase II Digestive... tract SRX112957,SRX143802 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.05.RNA_Polymerase_II.AllCell.bed ...

  8. File list: Pol.Dig.50.RNA_Polymerase_III.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.50.RNA_Polymerase_III.AllCell mm9 RNA polymerase RNA Polymerase III Digesti...ve tract http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.50.RNA_Polymerase_III.AllCell.bed ...

  9. File list: ALL.Dig.20.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.Jejunum mm9 All antigens Digestive tract Jejunum SRX1029569,SRX102...9566,SRX1029567,SRX1029568,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.20.AllAg.Jejunum.bed ...

  10. File list: ALL.Dig.05.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Jejunum mm9 All antigens Digestive tract Jejunum SRX1029566,SRX102...9569,SRX1029567,SRX1029568,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.05.AllAg.Jejunum.bed ...

  11. File list: ALL.Dig.50.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.Jejunum mm9 All antigens Digestive tract Jejunum SRX1029566,SRX102...9569,SRX1029567,SRX1029568,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.50.AllAg.Jejunum.bed ...

  12. File list: ALL.Dig.10.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Jejunum mm9 All antigens Digestive tract Jejunum SRX1029566,SRX102...9569,SRX1029568,SRX1029567,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.10.AllAg.Jejunum.bed ...

  13. File list: Unc.Dig.50.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.50.AllAg.Jejunum mm9 Unclassified Digestive tract Jejunum SRX1029566,SRX102...9569,SRX1029567,SRX1029568,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.50.AllAg.Jejunum.bed ...

  14. File list: Unc.Dig.20.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.20.AllAg.Jejunum mm9 Unclassified Digestive tract Jejunum SRX1029569,SRX102...9566,SRX1029567,SRX1029568,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.20.AllAg.Jejunum.bed ...

  15. File list: Unc.Dig.05.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.05.AllAg.Jejunum mm9 Unclassified Digestive tract Jejunum SRX1029566,SRX102...9569,SRX1029567,SRX1029568,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.05.AllAg.Jejunum.bed ...

  16. File list: Unc.Dig.10.AllAg.Jejunum [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.10.AllAg.Jejunum mm9 Unclassified Digestive tract Jejunum SRX1029566,SRX102...9569,SRX1029568,SRX1029567,SRX1029565 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.10.AllAg.Jejunum.bed ...

  17. File list: His.Dig.20.H2APERIODZ.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available His.Dig.20.H2APERIODZ.AllCell hg19 Histone H2A.Z Digestive tract SRX610758,SRX62566...5,SRX625659,SRX610766 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.20.H2APERIODZ.AllCell.bed ...

  18. File list: InP.Dig.20.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.20.AllAg.Colon mm9 Input control Digestive tract Colon SRX276118,SRX376980,...SRX376981,SRX376973 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.20.AllAg.Colon.bed ...

  19. File list: InP.Dig.10.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.AllAg.Colon mm9 Input control Digestive tract Colon SRX276118,SRX376973,...SRX376980,SRX376981 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.10.AllAg.Colon.bed ...

  20. File list: ALL.Dig.05.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Colon hg19 All antigens Digestive tract Colon SRX213493,SRX213496,...38,SRX142120,SRX863778,SRX055154,SRX136955,SRX157645,SRX263914 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.05.AllAg.Colon.bed ...

  1. File list: Oth.Dig.10.AllAg.Intestinal_villus [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.10.AllAg.Intestinal_villus mm9 TFs and others Digestive tract Intestinal vi...X871677 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.10.AllAg.Intestinal_villus.bed ...

  2. File list: Oth.Dig.20.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available X424010 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.20.AllAg.KYSE-150.bed ... ...Oth.Dig.20.AllAg.KYSE-150 hg19 TFs and others Digestive tract KYSE-150 SRX424011,SR

  3. File list: His.Dig.20.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ,SRX424015,SRX424013,SRX424014 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.20.AllAg.KYSE-150.bed ... ...His.Dig.20.AllAg.KYSE-150 hg19 Histone Digestive tract KYSE-150 SRX424016,SRX424017

  4. File list: Oth.Dig.05.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 77131 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.AllAg.KYSE-70.bed ... ...Oth.Dig.05.AllAg.KYSE-70 hg19 TFs and others Digestive tract KYSE-70 SRX277132,SRX2

  5. File list: ALL.Dig.10.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 130,SRX277131 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.10.AllAg.KYSE-70.bed ... ...ALL.Dig.10.AllAg.KYSE-70 hg19 All antigens Digestive tract KYSE-70 SRX277132,SRX277

  6. File list: ALL.Dig.10.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 24011,SRX424012,SRX424015,SRX424017,SRX424010,SRX424013,SRX424014 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.10.AllAg.KYSE-150.bed ... ...ALL.Dig.10.AllAg.KYSE-150 hg19 All antigens Digestive tract KYSE-150 SRX424016,SRX4

  7. File list: Oth.Dig.50.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 77132 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.50.AllAg.KYSE-70.bed ... ...Oth.Dig.50.AllAg.KYSE-70 hg19 TFs and others Digestive tract KYSE-70 SRX277131,SRX2

  8. File list: ALL.Dig.50.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 132,SRX277130 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.50.AllAg.KYSE-70.bed ... ...ALL.Dig.50.AllAg.KYSE-70 hg19 All antigens Digestive tract KYSE-70 SRX277131,SRX277

  9. File list: ALL.Dig.20.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 131,SRX277130 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.20.AllAg.KYSE-70.bed ... ...ALL.Dig.20.AllAg.KYSE-70 hg19 All antigens Digestive tract KYSE-70 SRX277132,SRX277

  10. File list: Oth.Dig.20.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 77131 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.20.AllAg.KYSE-70.bed ... ...Oth.Dig.20.AllAg.KYSE-70 hg19 TFs and others Digestive tract KYSE-70 SRX277132,SRX2

  11. File list: Oth.Dig.05.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available X424010 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.AllAg.KYSE-150.bed ... ...Oth.Dig.05.AllAg.KYSE-150 hg19 TFs and others Digestive tract KYSE-150 SRX424011,SR

  12. File list: ALL.Dig.05.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 132,SRX277131 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.05.AllAg.KYSE-70.bed ... ...ALL.Dig.05.AllAg.KYSE-70 hg19 All antigens Digestive tract KYSE-70 SRX277130,SRX277

  13. File list: ALL.Dig.05.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 24016,SRX424012,SRX424015,SRX424017,SRX424010,SRX424013,SRX424014 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.05.AllAg.KYSE-150.bed ... ...ALL.Dig.05.AllAg.KYSE-150 hg19 All antigens Digestive tract KYSE-150 SRX424011,SRX4

  14. File list: His.Dig.50.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ,SRX424016,SRX424013,SRX424014 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/His.Dig.50.AllAg.KYSE-150.bed ... ...His.Dig.50.AllAg.KYSE-150 hg19 Histone Digestive tract KYSE-150 SRX424017,SRX424015

  15. File list: Oth.Dig.10.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available X424010 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.10.AllAg.KYSE-150.bed ... ...Oth.Dig.10.AllAg.KYSE-150 hg19 TFs and others Digestive tract KYSE-150 SRX424011,SR

  16. File list: ALL.Dig.20.AllAg.KYSE-150 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 24012,SRX424011,SRX424017,SRX424010,SRX424015,SRX424013,SRX424014 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.20.AllAg.KYSE-150.bed ... ...ALL.Dig.20.AllAg.KYSE-150 hg19 All antigens Digestive tract KYSE-150 SRX424016,SRX4

  17. File list: DNS.Dig.05.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.05.AllAg.Colon hg19 DNase-seq Digestive tract Colon SRX100984,SRX089259,SRX...RX204363,SRX089272,SRX055154 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.05.AllAg.Colon.bed ...

  18. File list: DNS.Dig.20.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.20.AllAg.Colon hg19 DNase-seq Digestive tract Colon SRX089252,SRX100958,SRX...RX089272,SRX055159,SRX055154 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.20.AllAg.Colon.bed ...

  19. File list: DNS.Dig.10.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.10.AllAg.Colon hg19 DNase-seq Digestive tract Colon SRX100984,SRX089252,SRX...RX089272,SRX055159,SRX055154 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.10.AllAg.Colon.bed ...

  20. File list: DNS.Dig.50.AllAg.Colon [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.50.AllAg.Colon hg19 DNase-seq Digestive tract Colon SRX089252,SRX100958,SRX...RX089272,SRX055159,SRX055154 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.50.AllAg.Colon.bed ...

  1. File list: DNS.Dig.20.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.20.AllAg.Intestinal_crypt mm9 DNase-seq Digestive tract Intestinal crypt ht...tp://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.20.AllAg.Intestinal_crypt.bed ...

  2. File list: InP.Dig.05.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.05.AllAg.Intestinal_crypt mm9 Input control Digestive tract Intestinal cryp...t http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.05.AllAg.Intestinal_crypt.bed ...

  3. File list: NoD.Dig.20.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.20.AllAg.Intestinal_crypt mm9 No description Digestive tract Intestinal cry...pt http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/NoD.Dig.20.AllAg.Intestinal_crypt.bed ...

  4. File list: Pol.Dig.10.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.10.AllAg.Intestinal_crypt mm9 RNA polymerase Digestive tract Intestinal cry...pt http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.10.AllAg.Intestinal_crypt.bed ...

  5. File list: InP.Dig.10.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.AllAg.Intestinal_crypt mm9 Input control Digestive tract Intestinal cryp...t http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.10.AllAg.Intestinal_crypt.bed ...

  6. File list: InP.Dig.50.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.50.AllAg.Intestinal_crypt mm9 Input control Digestive tract Intestinal cryp...t http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.50.AllAg.Intestinal_crypt.bed ...

  7. File list: DNS.Dig.50.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.50.AllAg.Intestinal_crypt mm9 DNase-seq Digestive tract Intestinal crypt ht...tp://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.50.AllAg.Intestinal_crypt.bed ...

  8. File list: ALL.Dig.20.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.Intestinal_crypt mm9 All antigens Digestive tract Intestinal crypt... SRX871676,SRX871672,SRX871675,SRX871671 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.20.AllAg.Intestinal_crypt.bed ...

  9. File list: InP.Dig.20.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.20.AllAg.Intestinal_crypt mm9 Input control Digestive tract Intestinal cryp...t http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.20.AllAg.Intestinal_crypt.bed ...

  10. File list: ALL.Dig.50.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.Intestinal_crypt mm9 All antigens Digestive tract Intestinal crypt... SRX871671,SRX871676,SRX871675,SRX871672 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.50.AllAg.Intestinal_crypt.bed ...

  11. File list: Oth.Dig.05.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Intestinal_crypt mm9 TFs and others Digestive tract Intestinal cry...pt SRX871676,SRX871675,SRX871671,SRX871672 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.05.AllAg.Intestinal_crypt.bed ...

  12. File list: NoD.Dig.10.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.10.AllAg.Intestinal_crypt mm9 No description Digestive tract Intestinal cry...pt http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/NoD.Dig.10.AllAg.Intestinal_crypt.bed ...

  13. File list: Pol.Dig.05.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.05.AllAg.Intestinal_crypt mm9 RNA polymerase Digestive tract Intestinal cry...pt http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.05.AllAg.Intestinal_crypt.bed ...

  14. File list: Pol.Dig.20.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.20.AllAg.Intestinal_crypt mm9 RNA polymerase Digestive tract Intestinal cry...pt http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.20.AllAg.Intestinal_crypt.bed ...

  15. File list: DNS.Dig.10.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.10.AllAg.Intestinal_crypt mm9 DNase-seq Digestive tract Intestinal crypt ht...tp://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.10.AllAg.Intestinal_crypt.bed ...

  16. File list: NoD.Dig.05.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.05.AllAg.Intestinal_crypt mm9 No description Digestive tract Intestinal cry...pt http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/NoD.Dig.05.AllAg.Intestinal_crypt.bed ...

  17. File list: ALL.Dig.10.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Intestinal_crypt mm9 All antigens Digestive tract Intestinal crypt... SRX871676,SRX871671,SRX871675,SRX871672 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.10.AllAg.Intestinal_crypt.bed ...

  18. File list: ALL.Dig.05.AllAg.Intestinal_crypt [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Intestinal_crypt mm9 All antigens Digestive tract Intestinal crypt... SRX871676,SRX871675,SRX871671,SRX871672 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.05.AllAg.Intestinal_crypt.bed ...

  19. File list: Oth.Dig.10.AllAg.KYSE-70 [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available 77131 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.10.AllAg.KYSE-70.bed ... ...Oth.Dig.10.AllAg.KYSE-70 hg19 TFs and others Digestive tract KYSE-70 SRX277132,SRX2

  20. File list: ALL.Dig.05.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Stomach hg19 All antigens Digestive tract Stomach SRX252720,SRX252...55162,SRX121286,SRX055202,SRX201194,SRX055185,SRX121291,SRX055192,SRX214043,SRX252726 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/ALL.Dig.05.AllAg.Stomach.bed ...

  1. File list: DNS.Dig.10.AllAg.Stomach [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.10.AllAg.Stomach hg19 DNase-seq Digestive tract Stomach SRX089271,SRX100995...91,SRX055192,SRX214043 http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/DNS.Dig.10.AllAg.Stomach.bed ...

  2. File list: ALL.Dig.05.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.05.AllAg.Intestinal_adenoma mm9 All antigens Digestive tract Intestinal adenoma... SRX648718,SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.05.AllAg.Intestinal_adenoma.bed ...

  3. File list: NoD.Dig.05.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.05.AllAg.Intestinal_adenoma mm9 No description Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/NoD.Dig.05.AllAg.Intestinal_adenoma.bed ...

  4. File list: ALL.Dig.20.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.20.AllAg.Intestinal_adenoma mm9 All antigens Digestive tract Intestinal adenoma... SRX648718,SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.20.AllAg.Intestinal_adenoma.bed ...

  5. File list: ALL.Dig.50.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.50.AllAg.Intestinal_adenoma mm9 All antigens Digestive tract Intestinal adenoma... SRX648718,SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.50.AllAg.Intestinal_adenoma.bed ...

  6. File list: NoD.Dig.10.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.10.AllAg.Intestinal_adenoma mm9 No description Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/NoD.Dig.10.AllAg.Intestinal_adenoma.bed ...

  7. File list: InP.Dig.05.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.05.AllAg.Intestinal_adenoma mm9 Input control Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.05.AllAg.Intestinal_adenoma.bed ...

  8. File list: Oth.Dig.05.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Intestinal_adenoma mm9 TFs and others Digestive tract Intestinal adenoma... SRX648718 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.05.AllAg.Intestinal_adenoma.bed ...

  9. File list: DNS.Dig.05.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.05.AllAg.Intestinal_adenoma mm9 DNase-seq Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.05.AllAg.Intestinal_adenoma.bed ...

  10. File list: Unc.Dig.50.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.50.AllAg.Intestinal_adenoma mm9 Unclassified Digestive tract Intestinal adenoma... SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.50.AllAg.Intestinal_adenoma.bed ...

  11. File list: NoD.Dig.20.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available NoD.Dig.20.AllAg.Intestinal_adenoma mm9 No description Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/NoD.Dig.20.AllAg.Intestinal_adenoma.bed ...

  12. File list: DNS.Dig.20.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.20.AllAg.Intestinal_adenoma mm9 DNase-seq Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.20.AllAg.Intestinal_adenoma.bed ...

  13. File list: ALL.Dig.10.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available ALL.Dig.10.AllAg.Intestinal_adenoma mm9 All antigens Digestive tract Intestinal adenoma... SRX648718,SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/ALL.Dig.10.AllAg.Intestinal_adenoma.bed ...

  14. File list: Unc.Dig.05.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.05.AllAg.Intestinal_adenoma mm9 Unclassified Digestive tract Intestinal adenoma... SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.05.AllAg.Intestinal_adenoma.bed ...

  15. File list: Pol.Dig.50.RNA_Polymerase_II.AllCell [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Pol.Dig.50.RNA_Polymerase_II.AllCell mm9 RNA polymerase RNA Polymerase II Digestive... tract SRX112957,SRX143802 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Pol.Dig.50.RNA_Polymerase_II.AllCell.bed ...

  16. File list: Unc.Dig.10.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.10.AllAg.Intestinal_adenoma mm9 Unclassified Digestive tract Intestinal adenoma... SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.10.AllAg.Intestinal_adenoma.bed ...

  17. File list: Unc.Dig.20.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Unc.Dig.20.AllAg.Intestinal_adenoma mm9 Unclassified Digestive tract Intestinal adenoma... SRX648717 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Unc.Dig.20.AllAg.Intestinal_adenoma.bed ...

  18. File list: Oth.Dig.20.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.AllAg.Intestinal_adenoma mm9 TFs and others Digestive tract Intestinal adenoma... SRX648718 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.20.AllAg.Intestinal_adenoma.bed ...

  19. File list: InP.Dig.10.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.AllAg.Intestinal_adenoma mm9 Input control Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.10.AllAg.Intestinal_adenoma.bed ...

  20. File list: InP.Dig.50.AllAg.Intestinal_adenoma [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.50.AllAg.Intestinal_adenoma mm9 Input control Digestive tract Intestinal adenoma... http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/InP.Dig.50.AllAg.Intestinal_adenoma.bed ...

  1. File list: DNS.Dig.05.AllAg.Intestine,_Small [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available DNS.Dig.05.AllAg.Intestine,_Small mm9 DNase-seq Digestive tract Intestine, Small ht...tp://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/DNS.Dig.05.AllAg.Intestine,_Small.bed ...

  2. File list: InP.Dig.10.AllAg.Intestine,_Small [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available InP.Dig.10.AllAg.Intestine,_Small hg19 Input control Digestive tract Intestine, Small... http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/InP.Dig.10.AllAg.Intestine,_Small.bed ...

  3. File list: Oth.Dig.20.AllAg.Intestine,_Small [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.20.AllAg.Intestine,_Small mm9 TFs and others Digestive tract Intestine, Small...,SRX885790,SRX885799,SRX885798 http://dbarchive.biosciencedbc.jp/kyushu-u/mm9/assembled/Oth.Dig.20.AllAg.Intestine,_Small.bed ...

  4. File list: Oth.Dig.05.AllAg.Intestine,_Small [Chip-atlas[Archive

    Lifescience Database Archive (English)

    Full Text Available Oth.Dig.05.AllAg.Intestine,_Small hg19 TFs and others Digestive tract Intestine, Small... http://dbarchive.biosciencedbc.jp/kyushu-u/hg19/assembled/Oth.Dig.05.AllAg.Intestine,_Small.bed ...

  5. File list: NoD.Dig.20.AllAg.Intestine,_Small [Chip-atlas[Archive

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  14. The Asteroid Redirect Mission (ARM)

    Science.gov (United States)

    Abell, Paul; Gates, Michele; Johnson, Lindley; Chodas, Paul; Mazanek, Dan; Reeves, David; Ticker, Ronald

    2016-07-01

    To achieve its long-term goal of sending humans to Mars, the National Aeronautics and Space Administration (NASA) plans to proceed in a series of incrementally more complex human spaceflight missions. Today, human flight experience extends only to Low-Earth Orbit (LEO), and should problems arise during a mission, the crew can return to Earth in a matter of minutes to hours. The next logical step for human spaceflight is to gain flight experience in the vicinity of the Moon. These cis-lunar missions provide a "proving ground" for the testing of systems and operations while still accommodating an emergency return path to the Earth that would last only several days. Cis-lunar mission experience will be essential for more ambitious human missions beyond the Earth-Moon system, which will require weeks, months, or even years of transit time. In addition, NASA has been given a Grand Challenge to find all asteroid threats to human populations and know what to do about them. Obtaining knowledge of asteroid physical properties combined with performing technology demonstrations for planetary defense provide much needed information to address the issue of future asteroid impacts on Earth. Hence the combined objectives of human exploration and planetary defense give a rationale for the Asteroid Re-direct Mission (ARM). Mission Description: NASA's ARM consists of two mission segments: 1) the Asteroid Redirect Robotic Mission (ARRM), the first robotic mission to visit a large (greater than ~100 m diameter) near-Earth asteroid (NEA), collect a multi-ton boulder from its surface along with regolith samples, demonstrate a planetary defense technique, and return the asteroidal material to a stable orbit around the Moon; and 2) the Asteroid Redirect Crewed Mission (ARCM), in which astronauts will take the Orion capsule to rendezvous and dock with the robotic vehicle, conduct multiple extravehicular activities to explore the boulder, and return to Earth with samples. NASA's proposed

  15. Migration of Near Earth Asteroid to Jovian-Crosser Asteroid:Case Study 3552 Don Quixote

    OpenAIRE

    Siregar, Suryadi

    2010-01-01

    It is generally recognized that main-belt asteroids (MBAs) and nuclei of extinct comets are the two main sources for the Near-Earth-Asteroids (NEAs). Theoretical studies of NEAs dynamics and numerical modelling of their orbital motions showed that the resonance mechanism for supplying NEAs is quite sufficient to sustain this population. Asteroid 1983 SA, also known as 3552 Don Quixote, is one of Near Earth Asteroids (NEAs) and the most probable candidates for NEAs of the cometary origin. In t...

  16. Selecting asteroids for a targeted spectroscopic survey

    CERN Document Server

    Oszkiewicz, D A; Tomov, T; Birlan, M; Geier, S; Penttilä, A; Polińska, M

    2014-01-01

    Asteroid spectroscopy reflects surface mineralogy. There are few thousand asteroids whose surfaces have been observed spectrally. Determining the surface properties of those objects is important for many practical and scientific applications, such as for example developing impact deflection strategies or studying history and evolution of the Solar System and planet formation. The aim of this study is to develop a pre-selection method that can be utilized in searching for asteroids of any taxonomic complex. The method could then be utilized im multiple applications such as searching for the missing V-types or looking for primitive asteroids. We used the Bayes Naive Classifier combined with observations obtained in the course of the Sloan Digital Sky Survey and the Wide-field Infrared Survey Explorer surveys as well as a database of asteroid phase curves for asteroids with known taxonomic type. Using the new classification method we have selected a number of possible V-type candidates. Some of the candidates we...

  17. Earth-crossing asteroids - New discoveries

    Science.gov (United States)

    Helin, E. F.

    1982-01-01

    An earth-crossing asteroid is an asteroid whose orbit will intersect the orbit of the earth as a result of secular perturbations. Astronomical observations have led to the discovery of 43 earth-crossing asteroids during the last fifty years. Nearly sixty percent of these were found in the decade 1971-1981. Noteworthy results of the last decade are discussed, taking into account the Aten asteroids, accidental rediscoveries, asteroids of possible cometary origin, candidates for rendezvous and sample return missions, and populations and collision rates with earth. The observed earth-crossing asteroids are listed in a table, and the orbits of earth, Mars, and four Atens projected on ecliptic plane are shown.

  18. Asteroids prospective energy and material resources

    CERN Document Server

    2013-01-01

    The Earth has limited material and energy resources while these resources in space are virtually unlimited. Further development of humanity will require going beyond our planet and exploring of extraterrestrial resources and sources of unlimited power.   Thus far, all missions to asteroids have been motivated by scientific exploration. However, given recent advancements in various space technologies, mining asteroids for resources is becoming ever more feasible. A significant portion of asteroids value is derived from their location; the required resources do not need to be lifted at a great expense from the surface of the Earth.   Resources derived from Asteroid not only can be brought back to Earth but could also be used to sustain human exploration of space and permanent settlements in space.   This book investigates asteroids' prospective energy and material resources. It is a collection of topics related to asteroid exploration, and utilization. It presents past and future technologies and solutions t...

  19. Anchoring a lander on an asteroid using foam stabilization Project

    Data.gov (United States)

    National Aeronautics and Space Administration — NASA has proposed several missions to land a craft on an asteroid and potentially to return samples from it. While large asteroids in the asteroid belt can exhibit...

  20. Families classification including multiopposition asteroids

    Science.gov (United States)

    Milani, Andrea; Spoto, Federica; Knežević, Zoran; Novaković, Bojan; Tsirvoulis, Georgios

    2016-01-01

    In this paper we present the results of our new classification of asteroid families, upgraded by using catalog with > 500,000 asteroids. We discuss the outcome of the most recent update of the family list and of their membership. We found enough evidence to perform 9 mergers of the previously independent families. By introducing an improved method of estimation of the expected family growth in the less populous regions (e.g. at high inclination) we were able to reliably decide on rejection of one tiny group as a probable statistical fluke. Thus we reduced our current list to 115 families. We also present newly determined ages for 6 families, including complex 135 and 221, improving also our understanding of the dynamical vs. collisional families relationship. We conclude with some recommendations for the future work and for the family name problem.

  1. Regular Motions of Resonant Asteroids

    Science.gov (United States)

    Ferraz-Mello, S.

    1990-11-01

    RESUMEN. Se revisan resultados analiticos relativos a soluciones regulares del problema asteroidal eliptico promediados en la vecindad de una resonancia con jupiten Mencionamos Ia ley de estructura para libradores de alta excentricidad, la estabilidad de los centros de liberaci6n, las perturbaciones forzadas por la excentricidad de jupiter y las 6rbitas de corotaci6n. ABSTRAC This paper reviews analytical results concerning the regular solutions of the elliptic asteroidal problem averaged in the neighbourhood of a resonance with jupiter. We mention the law of structure for high-eccentricity librators, the stability of the libration centers, the perturbations forced by the eccentricity ofjupiter and the corotation orbits. Key words: ASThROIDS

  2. Stabilities of asteroid orbits in resonances

    Institute of Scientific and Technical Information of China (English)

    2002-01-01

    A map of the asteroid motion is studied carefully. An exponential diffusion law in the chaotic sea and an algebraic law in the mixed region are observed. The effects of perturbations on diffusion are also discussed. The fixed points, their stabilities and the diffusion properties of the map give qualitative explanations of the distribution of asteroids, i.e. the depletion and accumulation of asteroids in the outer main belt, particularly in the first order mean motion resonances with Jupiter.

  3. Asteroid Evolution: Role of Geotechnical Properties

    CERN Document Server

    Sánchez, Paul

    2015-01-01

    This paper presents a brief review and latest results of the work that has been carried out by the Planetary Science community in order to understand that role of the geotechnical properties of granular asteroids (commonly known as "rubble-pile" asteroids) in their formation, evolution and possible disruption. As such, we will touch in aspects of the theoretical and numerical tools that have been used with this objective and how the obtained results compare to the observed asteroids.

  4. ADAM: All-Data Asteroid Modeling

    Science.gov (United States)

    Viikinkoski, Matti; Kaasalainen, Mikko; Durech, Josef

    2015-02-01

    ADAM (All-Data Asteroid Modeling) models asteroid shape reconstruction from observations. Developed in MATLAB with core routines in C, its features include general nonconvex and non-starlike parametric 3D shape supports and reconstruction of asteroid shape from any combination of lightcurves, adaptive optics images, HST/FGS data, disk-resolved thermal images, interferometry, and range-Doppler radar images. ADAM does not require boundary contour extraction for reconstruction and can be run in parallel.

  5. Exospheres from Asteroids to Planets

    Science.gov (United States)

    Killen, Rosemary M.; Burger, Matthew H.; Farrell, William M.; DREAM2

    2016-10-01

    The study of exospheres can help us understand the long-term loss of volatiles from planetary bodies due to interactions of planets, satellites, and small bodies with the interplanetary medium (solar wind, meteors, and dust), solar radiation, internal forces including diffusion and outgassing, and surface effects like sticking and chemistry. Recent evidence for water and OH on the moon has spurred interest in processes involving chemistry and sequestration of volatile species at the poles and in voids. In recent years, NASA has sent spacecraft to asteroids including Vesta and Ceres, and ESA sent Rosetta to the asteroids Lutetia and Steins. OSIRIS-REX will return a sample from a primitive asteroid, Bennu, to Earth. It is possible that a Phobos-Deimos flyby will be a precursor to a manned mission to Mars. Exospheric particles are derived from the surface and to some extent from interplanetary dust and meteoroids. By comparing the exospheric compositions before and after major meteor shower events it may be possible to determine the extent to which the exosphere reflects the surface composition. Observation of an escaping exosphere, termed a corona, is challenging. We therefore have embarked on a parametrical study of exospheres as a function of basic controlling parameters such as the mass of the primary object, mass of the exospheric species, heliocentric distance, rotation rate of the primary, composition of the body (asteroid type or icy body). These parameters will be useful for mission planning as well as quick look data to determine the size and location of bodies likely to retain their exospheres and observability of exospheric species. We will also consider the sizes of small clusters that may be gravitationally bound to small bodies such as Phobos. In addition, it is of interest to be able to determine the extent of contamination of the pristine exosphere due to the spacecraft sent to make measurements, and the effect on the measurements of outgassing in the

  6. Asteroid Models from Multiple Data Sources

    Science.gov (United States)

    Durech, J.; Carry, B.; Delbo, M.; Kaasalainen, M.; Viikinkoski, M.

    In the past decade, hundreds of asteroid shape models have been derived using the lightcurve inversion method. At the same time, a new framework of three-dimensional shape modeling based on the combined analysis of widely different data sources -- such as optical lightcurves, disk-resolved images, stellar occultation timings, mid-infrared thermal radiometry, optical interferometry, and radar delay-Doppler data -- has been developed. This multi-data approach allows the determination of most of the physical and surface properties of asteroids in a single, coherent inversion, with spectacular results. We review the main results of asteroid lightcurve inversion and also recent advances in multi-data modeling. We show that models based on remote sensing data were confirmed by spacecraft encounters with asteroids, and we discuss how the multiplication of highly detailed three-dimensional models will help to refine our general knowledge of the asteroid population. The physical and surface properties of asteroids, i.e., their spin, three-dimensional shape, density, thermal inertia, and surface roughness, are among the least known of all asteroid properties. Apart from the albedo and diameter, we have access to the whole picture for only a few hundreds of asteroids. These quantities are nevertheless very important to understand, as they affect the nongravitational Yarkovsky effect responsible for meteorite delivery to Earth, as well as the bulk composition and internal structure of asteroids.

  7. Collisional and Rotational Disruption of Asteroids

    Science.gov (United States)

    Walsh, Kevin J.; Michel, Patrick; Richardson, Derek C.

    2011-02-01

    Asteroids are leftover pieces from the era of planet formation that help us understand conditions in the early Solar System. Unlike larger planetary bodies that were subject to global thermal modification during and subsequent to their formation, these small bodies have kept at least some unmodified primordial material from the solar nebula. However, the structural properties of asteroids have been modified considerably since their formation. Thus, we can find among them a great variety of physical configurations and dynamical histories. In fact, with only a few possible exceptions, all asteroids have been modified or completely disrupted many times during the age of the Solar System. This picture is supported by data from space mission encounters with asteroids that show much diversity of shape, bulk density, surface morphology, and other features. Moreover, the gravitational attraction of these bodies is so small that some physical processes occur in a manner far removed from our common experience on Earth. Thus, each visit to a small body has generated as many questions as it has answered. In this review we discuss the current state of research into asteroid disruption processes, focusing on collisional and rotational mechanisms. We find that recent advances in modeling catastrophic disruption by collisions have provided important insights into asteroid internal structures and a deeper understanding of asteroid families. Rotational disruption, by tidal encounters or thermal effects, is responsible for altering many smaller asteroids, and is at the origin of many binary asteroids and oddly shaped bodies.

  8. 基于 CATIA 的马铃薯挖掘铲参数化建模%Potato Digging Blade Parametric Modeling Method Based on CATIA

    Institute of Scientific and Technical Information of China (English)

    侯占峰; 王春光; 薛晶

    2014-01-01

    论述了马铃薯挖掘机关键部件挖掘铲的设计方法,并基于土壤与铲体作用力学分析建立了挖掘铲牵引阻力数学模型,最终确定了挖掘铲设计参数。同时,详细地阐述了基于 CATIA 的挖掘铲三维参数化建模的基本方法。%The principal parts design of potato harvester and the determination of parameters were stated in this article . The draught resistance mathematic model was set up based on dynamics analysis of digging blade and soil .At last the de-sign parameters of digging blade were confirmed .At the same time , a study is carried out upon three-dimensional para-metric modeling method and its technology based on CATIA , the basic method and general steps of potato digging blade 3-D parametric modeling are expounded in detail .

  9. Is the reddening of asteroids still a dilemma?

    Science.gov (United States)

    Moretti, P. F.:; Maras, A.; Folco, L.

    The association of the most abundant population of meteorites the ordinary chondrites and their parent bodies through the comparison of their reflected spectra has been a long debate In fact many of the asteroids show reddened spectra when observed in the visible and near-infrared range Gaffey 1976 Cloutis et al 1990 This reddening first observed in lunar mature soils has been demonstrated to be caused by the presence of metallic nano-particles Pieters et al 2000 Noble et al 2004 Though laboratory experiments reproduced the formation of such npFe as due to the vaporization of Fe-bearing silicates caused by the bombardment of micro meteoroids Sasaki et al 2001 the close-up observations of S-type asteroids obtained by the NEAR mission proposed a new mystery to be solved In fact if the continuous exposition to the space conditions should in principle darken and redden the surface of asteroids the slopes of the Psyche crater on Eros shows redder but brighter spectra when compared to the proposed associated meteorites Clark et al 2001 This result asked for a mechanism capable to redden much more than darken Very recently an alternative process has been suggested for surface alteration of airless bodies In fact metallic nano-particles have been demonstrated to be formed in Fe-Ni regions of ordinary chondrites where shock-induced transformation occurred Moretti et al 2005 Even if this last mechanism is capable to redden almost instantaneously localized regions on asteroids surfaces the distribution of the spectral slopes

  10. Asteroid regoliths: The development of a database

    Science.gov (United States)

    Graps, A.

    2014-07-01

    There is a variety of evidence that asteroids, including the smallest asteroids, possess regoliths. This layer is our interface between the asteroid's interior physical processes and its exterior manifestation. By going beyond the remote study of asteroids with Hayabusa's brief touchdown onto Itokowa's surface, scientists, engineers, mission planners have new immediate questions and concerns about the asteroid regolith. For example: What if some asteroid surface features are transient due to dust transport? What are the risks about electrostatically sticky dust? Which alteration process (impact cratering, tectonics, shaking, dust levitation, and space weathering) can best explain the regolith properties of a particular asteroid? To address these questions, a method has been developed which will lead to a database of asteroid regolith properties to aid asteroid investigators. The method is illustrated in the flowchart below. Three types of information is included: spacecraft-based in-situ data, laboratory-based meteorite samples, and telescopic remote data provide a system of cross-checking to increase the accuracy and the probability of gaining new information. Theoretical studies can provide additional cross-checking. A critical perspective, included here, is the assignment of the spatial scales where the bulk density and porosity of an asteroid is related to the average density and porosity of its constituent rocks, which is further distinguished from the average density of the mineral assemblages within the rocks. This presentation will step through the method and provide first regolith database results of the regolith properties: grain density, size, thermal conductivity, porosity, and volume filling factor for the asteroids (1)~Ceres, (2)~Pallas, (21)~Lutetia, and (4)~Vesta.

  11. Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey

    Science.gov (United States)

    Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; Ishihara, Daisuke; Kataza, Hirokazu; Takita, Satoshi; Oyabu, Shinki; Ueno, Munetaka; Matsuhara, Hideo; Onaka, Takashi

    2011-10-01

    We present the results of an unbiased asteroid survey in the mid-infrared wavelength region with the Infrared Camera (IRC) on board the Japanese infrared satellite AKARI. About 20% of the point source events recorded in the AKARI All-Sky Survey observations are not used for the IRC Point Source Catalog (IRC-PSC) in its production process because of a lack of multiple detection by position. Asteroids, which are moving objects on the celestial sphere, remain in these ``residual events''. We identify asteroids out of the residual events by matching them with the positions of known asteroids. For the identified asteroids, we calculate the size and albedo based on the Standard Thermal Model. Finally we have a new brand of asteroid catalog, named the Asteroid Catalog Using AKARI (AcuA), which contains 5120 objects, about twice as many as the IRAS asteroid catalog. The catalog objects comprise 4953 main belt asteroids, 58 near-Earth asteroids, and 109 Jovian Trojan asteroids. The catalog is publicly available via the Internet.

  12. Migration of Near Earth Asteroid to Jovian-Crosser Asteroid:Case Study 3552 Don Quixote

    CERN Document Server

    Siregar, Suryadi

    2010-01-01

    It is generally recognized that main-belt asteroids (MBAs) and nuclei of extinct comets are the two main sources for the Near-Earth-Asteroids (NEAs). Theoretical studies of NEAs dynamics and numerical modelling of their orbital motions showed that the resonance mechanism for supplying NEAs is quite sufficient to sustain this population. Asteroid 1983 SA, also known as 3552 Don Quixote, is one of Near Earth Asteroids (NEAs) and the most probable candidates for NEAs of the cometary origin. In this work, an investigation on the evolution of the orbit is done by using the SWIFT subroutine package, where the gravitational perturbations of eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune are considered. Migration of asteroid 3552 Don Quixote from Near Earth Asteroids (NEAs) to Jovian-crosser asteroid is found.

  13. Discontinuous Inter-Granular Separations (DIGS) in the Gas Nitride Layer of ISS Race Rings

    Science.gov (United States)

    Figert, John; Dasgupta, Rajib; Martinez, James

    2010-01-01

    The starboard solar alpha rotary joint (SARJ) race ring on the International space station (ISS) failed due to severe spalling of the outer diameter, 45 degree (outer canted) nitrided surface. Subsequent analysis at NASA-KSC revealed that almost all of the debris generated due to the failure was nitrided 15-5 stainless steel. Subsequent analysis of the nitride control coupons (NCC) at NASA-JSC revealed the presence of discontinuous inter-granular separations (DIGS) in the gas nitride layer. These DIGS were present in the inter-granular networking located in the top 2 mils of the nitride layer. The manufacturer's specification requires the maximum white structure to be 0.0003 inches and intergranular networking below the allowable white structure depth to be cause for rejection; a requirement that the NCCs did not meet. Subsequent testing and analysis revealed that lower DIGS content significantly lowered the probability of nitride spalling in simulated, dry condition runs. One batch of nitride samples with DIGS content similar to the port SARJ (did not fail on orbit) which exhibited almost no nitride spalling after being run on one test rig. Another batch of nitride samples with DIGS content levels similar to the starboard SARJ exhibited significant nitride spalling on the same test rig with the same load under dry conditions. Although DIGS were not the root cause of starboard race ring failure, testing indicates that increased DIGS reduced the robustness of the gas nitride layer under dry operating conditions.

  14. Organic matter on asteroid 130 Elektra

    Science.gov (United States)

    Cruikshank, D. P.; Brown, R. H.

    1987-01-01

    Infrared absorption spectra of a low-albedo water-rich asteroid appear to show a weak 3.4-micrometer carbon-hydrogen stretching mode band, which suggests the presence of hydrocarbons on asteroid 130 Elektra. The organic extract from the primitive carbonaceous chondritic Murchison meteorite shows similar spectral bands.

  15. Spectroscopy of near-Earth asteroids

    DEFF Research Database (Denmark)

    Michelsen, René; Nathues, Andreas; Lagerkvist, Claes-Ingvar

    2006-01-01

    We present spectra and taxonomic classifications of 12 Near-Earth Asteroids (NEAs) and 2 inner Main Belt asteroids. The observations were carried out with the ESO 3.5 m NTT and the Danish 1.54 m telescope at La Silla, Chile. Eleven of the investigated NEAs belong to the S class while only one C-t...

  16. Spitzer Survey of the Karin Cluster Asteroids

    NARCIS (Netherlands)

    Harris, Alan W.; Mueller, M.; Lisse, C.; Cheng, A.; Osip, D.

    2007-01-01

    The Karin cluster is one of the youngest known families of main-belt asteroids, dating back to a collisional event only 5.8 Myr ago. Using the Spitzer Space Telescope we have sampled the thermal continua of 17 Karin cluster asteroids, down to the smallest members discovered so far, in order to deriv

  17. Loss of SynDIG1 Reduces Excitatory Synapse Maturation But Not Formation In Vivo

    Science.gov (United States)

    Kaur, Inderpreet; Liu, Xiao-Bo; Kirk, Lyndsey M.; Speca, David J.; McMahon, Samuel A.; Zito, Karen

    2016-01-01

    Abstract Modification of the strength of excitatory synaptic connections is a fundamental mechanism by which neural circuits are refined during development and learning. Synapse Differentiation Induced Gene 1 (SynDIG1) has been shown to play a key role in regulating synaptic strength in vitro. Here, we investigated the role of SynDIG1 in vivo in mice with a disruption of the SynDIG1 gene rather than use an alternate loxP-flanked conditional mutant that we find retains a partial protein product. The gene-trap insertion with a reporter cassette mutant mice shows that the SynDIG1 promoter is active during embryogenesis in the retina with some activity in the brain, and postnatally in the mouse hippocampus, cortex, hindbrain, and spinal cord. Ultrastructural analysis of the hippocampal CA1 region shows a decrease in the average PSD length of synapses and a decrease in the number of synapses with a mature phenotype. Intriguingly, the total synapse number appears to be increased in SynDIG1 mutant mice. Electrophysiological analyses show a decrease in AMPA and NMDA receptor function in SynDIG1-deficient hippocampal neurons. Glutamate stimulation of individual dendritic spines in hippocampal slices from SynDIG1-deficient mice reveals increased short-term structural plasticity. Notably, the overall levels of PSD-95 or glutamate receptors enriched in postsynaptic biochemical fractions remain unaltered; however, activity-dependent synapse development is strongly compromised upon the loss of SynDIG1, supporting its importance for excitatory synapse maturation. Together, these data are consistent with a model in which SynDIG1 regulates the maturation of excitatory synapse structure and function in the mouse hippocampus in vivo.

  18. The Compositional Structure of the Asteroid Belt

    CERN Document Server

    DeMeo, Francesca E; Walsh, Kevin J; Chapman, Clark R; Binzel, Richard P

    2015-01-01

    The past decade has brought major improvements in large-scale asteroid discovery and characterization with over half a million known asteroids and over 100,000 with some measurement of physical characterization. This explosion of data has allowed us to create a new global picture of the Main Asteroid Belt. Put in context with meteorite measurements and dynamical models, a new and more complete picture of Solar System evolution has emerged. The question has changed from "What was the original compositional gradient of the Asteroid Belt?" to "What was the original compositional gradient of small bodies across the entire Solar System?" No longer is the leading theory that two belts of planetesimals are primordial, but instead those belts were formed and sculpted through evolutionary processes after Solar System formation. This article reviews the advancements on the fronts of asteroid compositional characterization, meteorite measurements, and dynamical theories in the context of the heliocentric distribution of...

  19. Distribution and evolution of asteroid rotation rates

    Science.gov (United States)

    Dermott, S. F.; Murray, C. D.

    1984-01-01

    Data on the rotational characteristics of more than 300 asteroids are currently available, and it is now clear that the distribution of the rotation rates is nonrandom. A plot of rotation rate against asteroid diameter shows large dispersion but is distinctly V-shaped. The minimum of this curve at about 120 km may separate primordial asteroids from their collision products. There is also evidence that rotation rate depends on type classification, and weak evidence that it may also depend on family membership. Recent bias-free observations suggest that the marked rise of rotation rate with decreasing diameter D for those asteroids with D less than 120 km cannot be completely accounted for by observational-selection effects. A significantly large subset of the small asteroids have exceptionally long rotation periods suggestive of either a different nature and origin or a peculiar history. Models that have been proposed to account for these results are discussed.

  20. Asteroids in the Eccentrids meteor system

    Science.gov (United States)

    Terentjeva, A. K.; Barabanov, S. I.

    2016-09-01

    Among 11 673 of near-Earth objects (NEOs), 52 asteroids are identified, which, together with the Eccentrids meteor system, comprise a single population of small bodies of the Solar System with the smallest orbits of high eccentricity. Some features of this unique system of bodies are discussed in this paper. The distribution of perihelion longitudes is studied for the given group of asteroids and compared to that of the Aten asteroids, which are the most similar to the Eccentrids. The dependence is obtained of the character of perihelion longitude distribution on the eccentricities of the NEO orbits. Eight asteroid stream of the Eccentrids are found. The Eccentrids asteroids approaching the Earth's orbit along its whole length in their aphelia can pose a certain hazard for the Earth.

  1. On the Astrid asteroid family

    Science.gov (United States)

    Carruba, V.

    2016-09-01

    Among asteroid families, the Astrid family is peculiar because of its unusual inclination distribution. Objects at a ≃ 2.764 au are quite dispersed in this orbital element, giving the family a `crab-like' appearance. Recent works showed that this feature is caused by the interaction of the family with the s - sC nodal secular resonance with Ceres, that spreads the inclination of asteroids near its separatrix. As a consequence, the currently observed distribution of the vW component of terminal ejection velocities obtained from inverting Gauss equation is quite leptokurtic, since this parameter mostly depends on the asteroids inclination. The peculiar orbital configuration of the Astrid family can be used to set constraints on key parameters describing the strength of the Yarkovsky force, such as the bulk and surface density and the thermal conductivity of surface material. By simulating various fictitious families with different values of these parameters, and by demanding that the current value of the kurtosis of the distribution in vW be reached over the estimated lifetime of the family, we obtained that the thermal conductivity of Astrid family members should be ≃0.001 W m-1 K-1, and that the surface and bulk density should be higher than 1000 kg m-3. Monte Carlo methods simulating Yarkovsky and stochastic Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) evolution of the Astrid family show its age to be T = 140 ± 30 Myr old, in good agreement with estimates from other groups. Its terminal ejection velocity parameter is in the range V_{EJ}= 5^{+17}_{-5} m s-1. Values of VEJ larger than 25 m s-1 are excluded from constraints from the current inclination distribution.

  2. A Wide-Angle Camera for the Mobile Asteroid Surface Scout (MASCOT) on Hayabusa-2

    Science.gov (United States)

    Schmitz, N.; Koncz, A.; Jaumann, R.; Hoffmann, H.; Jobs, D.; Kachlicki, J.; Michaelis, H.; Mottola, S.; Pforte, B.; Schroeder, S.; Terzer, R.; Trauthan, F.; Tschentscher, M.; Weisse, S.; Ho, T.-M.; Biele, J.; Ulamec, S.; Broll, B.; Kruselburger, A.; Perez-Prieto, L.

    2014-04-01

    JAXA's Hayabusa-2 mission, an asteroid sample return mission, is scheduled for launch in December 2014, for a rendezvous with the C-type asteroid 1999 JU3 in 2018. MASCOT, the Mobile Asteroid Surface Scout [1], is a small lander, designed to deliver ground truth for the orbiter remote measurements, support the selection of sampling sites, and provide context for the returned samples.MASCOT's main objective is to investigate the landing site's geomorphology, the internal structure, texture and composition of the regolith (dust, soil and rocks), and the thermal, mechanical, and magnetic properties of the surface. MASCOT comprises a payload of four scientific instruments: camera, radiometer, magnetometer and hyper-spectral microscope. The camera (MASCOT CAM) was designed and built by DLR's Institute of Planetary Research, together with Airbus DS Germany.

  3. Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2014

    Science.gov (United States)

    Oey, Julian

    2016-01-01

    Photometric observations of a number of asteroids were done from Blue Mountains Observatory in 2014. The observations were made in support of the binary asteroid and asteroid pairs campaigns by Petr Pravec, and to obtain new data at favorable apparitions for asteroids with poorly defined lightcurves.

  4. Working Group Reports and Presentations: Asteroids

    Science.gov (United States)

    Lewis, John

    2006-01-01

    The study and utilization of asteroids will be an economical way to enable exploration of the solar system and extend human presence in space. There are thousands of near-earth objects (NEOs) that we will be able to reach. They offer resources, transportation, and exploration platforms, but also present a potential threat to civilization. Asteroids play a catastrophic role in the history of the Earth. Geological records indicate a regular history of massive impacts, which astronomical observations confirm is likely to continue with potentially devastating consequences. However, study and exploration of near earth asteroids can significantly increase advanced warning of an Earth impact, and potentially lead to the technology necessary to avert such a collision. Efforts to detect and prevent cataclysmic events would tend to foster and likely require international cooperation toward a unified goal of self-preservation. Exploration of asteroids will help us to understand our history and perhaps save our future. Besides the obvious and compelling scientific and security drivers for asteroid research and exploration, there are numerous engineering and industrial applications for near-term asteroid exploration. We have strong evidence that some asteroids are metal rich. Some are water and organic rich. They can be reached with a very low fuel cost compared to other solar system destinations. Once we reach them, there are efficient, simple extraction technologies available that would facilitate utilization. In addition, the costs of returning extracted resources from asteroids will be a fraction of the cost to return similar resources from the moon to Low Earth Orbit (LEO). These raw materials, extracted and shipped at relatively low cost, can be used to manufacture structures, fuel, and products which could be used to foster mankind s further exploration of the solar system. Asteroids also have the potential to offer transport to several destinations in the solar system

  5. Reconstructing HST Images of Asteroids

    Science.gov (United States)

    Storrs, A. D.; Bank, S.; Gerhardt, H.; Makhoul, K.

    2003-12-01

    We present reconstructions of images of 22 large main belt asteroids that were observed by Hubble Space Telescope with the Wide-Field/Planetary cameras. All images were restored with the MISTRAL program (Mugnier, Fusco, and Conan 2003) at enhanced spatial resolution. This is possible thanks to the well-studied and stable point spread function (PSF) on HST. We present some modeling of this process and determine that the Strehl ratio for WF/PC (aberrated) images can be improved to 130 ratio of 80 We will report sizes, shapes, and albedos for these objects, as well as any surface features. Images taken with the WFPC-2 instrument were made in a variety of filters so that it should be possible to investigate changes in mineralogy across the surface of the larger asteroids in a manner similar to that done on 4 Vesta by Binzel et al. (1997). Of particular interest are a possible water of hydration feature on 1 Ceres, and the non-observation of a constriction or gap between the components of 216 Kleopatra. Reduction of this data was aided by grant HST-GO-08583.08A from the Space Telescope Science Institute. References: Mugnier, L.M., T. Fusco, and J.-M. Conan, 2003. JOSA A (submitted) Binzel, R.P., Gaffey, M.J., Thomas, P.C., Zellner, B.H., Storrs, A.D., and Wells, E.N. 1997. Icarus 128 pp. 95-103

  6. Dynamical dispersal of primordial asteroid families

    Science.gov (United States)

    Brasil, P. I. O.; Roig, F.; Nesvorný, D.; Carruba, V.; Aljbaae, S.; Huaman, M. E.

    2016-03-01

    Many asteroid families are identified and well characterized all over the main asteroid belt. Interestingly, however, none of them are older than 4 Gyr. Many mechanisms have been proposed to disperse such old primordial asteroid families that presumably have existed, but only very few have really worked. Here we present a plausible mechanism for dispersing primordial asteroid families that is based on the 5-planet instability model known as jumping Jupiter. Using two different evolutions for the jumping-Jupiter model, we have numerically integrated orbits of eight putative primordial families. Our results show that the most important effect on the asteroid families' eccentricity and inclination dispersal is that of the secular resonances, in some cases associated with the mean motion resonances. As for the semimajor axes spreading we find that the principal effect is that of close encounters with the fifth giant planet whose orbit briefly overlaps with (part of) the main belt. Therefore, the existence of a fifth giant planet with the mass comparable with that of Uranus' or Neptune's could contribute in important ways to dispersal of the primordial asteroid families. To have that effect, the interloper planet should go into and considerably interact with the asteroids during the instability phase.

  7. Delivery of meteorites from the asteroid belt

    Science.gov (United States)

    Nolan, Michael Craig

    The process of the delivery of meteorites to the surface of the Earth from plausible source regions such as the asteroid belt is currently understood in general terms, but important uncertainties and conflicts remain to be resolved. Stochastic effects of the rare disruptions of large asteroids on the population of meteorite-sized Earth-crossing asteroids can change the flux and the proportions of compositional types in the infalling meteorite population. These changes can be significant in magnitude over timescales of 108 years. Changes of the order of 1 percent can be expected on timescales of 105-106 y, consistent with small differences between the Antarctic meteorites and modern falls. The magnitude of changes depends strongly on poorly-understood details of collisions. Asteroids 961 Gaspra and 243 Ida were recently imaged by the Galileo spacecraft. I use a numerical hydrocode model to examine the outcomes of various sire impacts into targets the sizes of these asteroids. A shock wave fractures the asteroid in advance of crater excavation flow; thus, for impactors larger than 100 m, impacting at 5.3 km s-1, tensile strength is unimportant in these bodies, whether they are initially intact or are 'rubble piles'. Because of the shock-induced fracture, impact results are controlled by gravity. Therefore these asteroids are much more resistant to catastrophic disruption than predicted by previous estimates, which had assumed that strength was controlling these processes for rock targets. Fracture of km-size asteroids is different from fracture in terrestrial experiments using few-cm targets. The composition distribution of delivered meteorites depends on the outcomes of such asteroid impacts.

  8. Reproductive ecology of Sichuan digging frogs (Microhylidae: Kaloula rugifera)

    OpenAIRE

    Wei Chen; Lina Ren; Dujuan He; Ying Wang; David Pike

    2015-01-01

    Abstract. We investigated the reproductive ecology of Sichuan digging frogs (Microhylidae: Kaloula rugifera) in Mianyang, China during the wet season of 2013. Male Sichuan digging frogs first appear at temporary ponds following the first heavy rain of the wet season and initiate calling. Females arrive at ponds shortly after males. Male frogs chorus extensively throughout the wet season during the evenings and nights following rainstorms. Female frogs leave the pond after laying eggs, and lik...

  9. A three-parameter asteroid taxonomy

    Science.gov (United States)

    Tedesco, Edward F.; Williams, James G.; Matson, Dennis L.; Veeder, Glenn J.; Gradie, Jonathan C.

    1989-01-01

    Broadband U, V, and x photometry together with IRAS asteroid albedos have been used to construct an asteroid classification system. The system is based on three parameters (U-V and v-x color indices and visual geometric albedo), and it is able to place 96 percent of the present sample of 357 asteroids into 11 taxonomic classes. It is noted that all but one of these classes are analogous to those previously found using other classification schemes. The algorithm is shown to account for the observational uncertainties in each of the classification parameters.

  10. A NEW DYNAMICAL POPULATION OF ASTEROIDS

    Directory of Open Access Journals (Sweden)

    T. Gallardo

    2009-01-01

    Full Text Available We have found approximately 1500 asteroids evolving in the exterior 1:2 resonance with Mars. Looking at the histogram of semimajor axes of the asteroids in the main belt the population can be distinguished as a peak at a ' 2:419 AU. Approximately 400 asteroids are librating around the asymmetric libration centers and about 700 are describing horseshoe trajectories. A strong secular perturbation due to Jupiter and due to Mars' eccentricity time evolution produces switching between libration centers and between librations and horseshoe trajectories. In spite of this strong secular e ect the population remains linked to the resonance over time scales of 108 - 109 years.

  11. Asteroids@home - A BOINC distributed computing project for asteroid shape reconstruction

    CERN Document Server

    Durech, Josef; Vanco, Radim

    2015-01-01

    We present the project Asteroids@home that uses distributed computing to solve the time-consuming inverse problem of shape reconstruction of asteroids. The project uses the Berkeley Open Infrastructure for Network Computing (BOINC) framework to distribute, collect, and validate small computational units that are solved independently at individual computers of volunteers connected to the project. Shapes, rotational periods, and orientations of the spin axes of asteroids are reconstructed from their disk-integrated photometry by the lightcurve inversion method.

  12. Near Earth Asteroids- Prospection, Orbit Modification and Mining

    Science.gov (United States)

    Grandl, W.; Bazso, A.

    2014-04-01

    The number of known Near Earth Asteroids (NEAs) has increased continuously during the last decades. Now we understand the role of asteroid impacts for the evolution of life on Earth. To ensure that mankind will survive in the long run, we have to face the "asteroid threat" seriously. On one hand we will have to develop methods of detection and deflection for Hazardous Asteroids, on the other hand we can use these methods to modify their orbits and exploit their resources. Rare-earth elements, rare metals like platinum group elements, etc. may be extracted more easily from NEAs than from terrestrial soil, without environmental pollution or political and social problems. In a first step NEAs, which are expected to contain resources like nickel-iron, platinum group metals or rare-earth elements, will be prospected by robotic probes. Then a number of asteroids with a minimum bulk density of 2 g/cm^3 and a diameter of 150 to 500 m will be selected for mining. Given the long duration of an individual mission time of 10-20 years, the authors propose a "pipeline" concept. While the observation of NEAs can be done in parallel, the precursor missions of the the next phase can be launched in short intervals, giving time for technical corrections and upgrades. In this way a continuous data flow is established and there are no idle times. For our purpose Potentially Hazardous Asteroids (PHAs) seem to be a favorable choice for the following reasons: They have frequent closeencounters to Earth, their minimum orbit intersection distance is less than 0.05 AU (Astronomic Units) and they have diameters exceeding 150 meters. The necessary velocity change (delta V) for a spaceship is below 12 km/s to reach the PHA. The authors propose to modify the orbits of the chosen PHAs by orbital maneuvers from solar orbits to stable Earth orbits beyond the Moon. To change the orbits of these celestial bodies it is necessary to develop advanced propulsion systems. They must be able to deliver high

  13. Water in Asteroid 4 Vesta

    Science.gov (United States)

    Taylor, G. J.

    2015-01-01

    Eucrite meteorites come from asteroid 4 Vesta, which was recently studied from orbit by NASA's Dawn mission. Adam Sarafian (Woods Hole Oceanographic Institute) and colleagues at Woods Hole, the University of Bristol, England, and the University of New Mexico measured the hydrogen concentration and deuterium/hydrogen (D/H) ratio in crystals of the mineral apatite (calcium phosphate) in eucrites. They found that the D/H ratio is in the same range as in carbonaceous chondrites, most samples of the Earth's mantle, and in samples of basaltic meteorites from Mars. Combined with measurements of the isotopic compositions of nitrogen and carbon, the data suggest that these volatile elements were added to Earth early in its history, probably during its formation. Other studies conclude that water with D/H like that in carbonaceous chondrites, Earth, Mars, and Vesta were likely inherited from interstellar ice that predates formation of the solar system.

  14. The Cratering History of Asteroid (21) Lutetia

    CERN Document Server

    Marchi, S; Vincent, J -B; Morbidelli, A; Mottola, S; Marzari, F; Kueppers, M; Besse, S; Thomas, N; Barbieri, C; Naletto, G; Sierks, H

    2011-01-01

    The European Space Agency's Rosetta spacecraft passed by the main belt asteroid (21) Lutetia the 10th July 2010. With its ~100km size, Lutetia is one of the largest asteroids ever imaged by a spacecraft. During the flyby, the on-board OSIRIS imaging system acquired spectacular images of Lutetia's northern hemisphere revealing a complex surface scarred by numerous impact craters, reaching the maximum dimension of about 55km. In this paper, we assess the cratering history of the asteroid. For this purpose, we apply current models describing the formation and evolution of main belt asteroids, that provide the rate and velocity distributions of impactors. These models, coupled with appropriate crater scaling laws, allow us to interpret the observed crater size-frequency distribution (SFD) and constrain the cratering history. Thanks to this approach, we derive the crater retention age of several regions on Lutetia, namely the time lapsed since their formation or global surface reset. We also investigate the influe...

  15. Mineralogy and Surface Composition of Asteroids

    CERN Document Server

    Reddy, Vishnu; Thomas, Cristina A; Moskovitz, Nicholas A; Burbine, Thomas H

    2015-01-01

    Methods to constrain the surface mineralogy of asteroids have seen considerable development during the last decade with advancement in laboratory spectral calibrations and validation of our interpretive methodologies by spacecraft rendezvous missions. This has enabled the accurate identification of several meteorite parent bodies in the main asteroid belt and helped constrain the mineral chemistries and abundances in ordinary chondrites and basaltic achondrites. With better quantification of spectral effects due to temperature, phase angle, and grain size, systematic discrepancies due to non-compositional factors can now be virtually eliminated for mafic silicate-bearing asteroids. Interpretation of spectrally featureless asteroids remains a challenge. This paper presents a review of all mineralogical interpretive tools currently in use and outlines procedures for their application.

  16. Collisional and Rotational Disruption of Asteroids

    CERN Document Server

    Walsh, Kevin J; Richardson, Derek C

    2009-01-01

    Asteroids are leftover pieces from the era of planet formation that help us understand conditions in the early Solar System. Unlike larger planetary bodies that were subject to global thermal modification during and subsequent to their formation, these small bodies have kept at least some unmodified primordial material from the solar nebula. However, the structural properties of asteroids have been modified considerably since their formation. Thus, we can find among them a great variety of physical configurations and dynamical histories. In fact, with only a few possible exceptions, all asteroids have been modified or completely disrupted many times during the age of the Solar System. This picture is supported by data from space mission encounters with asteroids that show much diversity of shape, bulk density, surface morphology, and other features. Moreover, the gravitational attraction of these bodies is so small that some physical processes occur in a manner far removed from our common experience on Earth....

  17. Asteroid Lightcurves from the Preston Gott Observatory

    Science.gov (United States)

    Clark, Maurice

    2012-04-01

    Results of analysis of CCD photometry observations obtained at the Preston Gott Observatory of asteroids 970 Primula, 3015 Candy, 3751 Kiang, 6746 Zagar, 7750 McEwen, 10046 Creighton, and 19251 Totziens are presented.

  18. Chelyabinsk: Portrait of an asteroid airburst

    Energy Technology Data Exchange (ETDEWEB)

    Kring, David A.; Boslough, Mark

    2014-09-01

    Video and audio from hundreds of smartphones and dashboard cameras combined with seismic, acoustic, and satellite measurements provide the first precise documentation of a 10 000-ton asteroid explosion.

  19. Chelyabinsk: Portrait of an asteroid airburst

    International Nuclear Information System (INIS)

    Video and audio from hundreds of smartphones and dashboard cameras combined with seismic, acoustic, and satellite measurements provide the first precise documentation of a 10 000-ton asteroid explosion

  20. Origins for the near-earth asteroids

    Science.gov (United States)

    Binzel, Richard P.; Xu, Shui; Bus, Schelte J.; Bowell, Edward

    1992-01-01

    Because of their short dynamical lifetimes, the population of near-earth asteroids (NEAs) must be resupplied. Two sources have been hypothesized: main-belt asteroids and extinct comet nuclei. A new survey of physical properties for less than 5 kilometers diameter main-belt asteroids reveals that their spin rate and shape distributions are similar to those of NEAs, as is fully consistent with a main-belt origin for most NEAs. Physical data on comet nuclei are limited. If the existing sample is representative of the comet population, analysis of the asteroid and comet samples constrains the fraction of comet nuclei to between 0 and 40 percent of the total NEA population.

  1. Asteroid models from the Lowell photometric database

    Science.gov (United States)

    Ďurech, J.; Hanuš, J.; Oszkiewicz, D.; Vančo, R.

    2016-03-01

    Context. Information about shapes and spin states of individual asteroids is important for the study of the whole asteroid population. For asteroids from the main belt, most of the shape models available now have been reconstructed from disk-integrated photometry by the lightcurve inversion method. Aims: We want to significantly enlarge the current sample (~350) of available asteroid models. Methods: We use the lightcurve inversion method to derive new shape models and spin states of asteroids from the sparse-in-time photometry compiled in the Lowell Photometric Database. To speed up the time-consuming process of scanning the period parameter space through the use of convex shape models, we use the distributed computing project Asteroids@home, running on the Berkeley Open Infrastructure for Network Computing (BOINC) platform. This way, the period-search interval is divided into hundreds of smaller intervals. These intervals are scanned separately by different volunteers and then joined together. We also use an alternative, faster, approach when searching the best-fit period by using a model of triaxial ellipsoid. By this, we can independently confirm periods found with convex models and also find rotation periods for some of those asteroids for which the convex-model approach gives too many solutions. Results: From the analysis of Lowell photometric data of the first 100 000 numbered asteroids, we derived 328 new models. This almost doubles the number of available models. We tested the reliability of our results by comparing models that were derived from purely Lowell data with those based on dense lightcurves, and we found that the rate of false-positive solutions is very low. We also present updated plots of the distribution of spin obliquities and pole ecliptic longitudes that confirm previous findings about a non-uniform distribution of spin axes. However, the models reconstructed from noisy sparse data are heavily biased towards more elongated bodies with high

  2. Digging into Inquiry-Based Earth Science Research

    Science.gov (United States)

    Schultz, Bryan; Yates, Crystal; Schultz, Jayne M.

    2008-01-01

    To help eighth-grade students experience the excitement of Earth science research, the authors developed an inquiry-based project in which students evaluated and cataloged their campus geology and soils. Following class discussions of rock-weathering and soil-forming processes, students worked in groups to excavate multiple soil pits in the school…

  3. An Early Warning System for Asteroid Impact

    CERN Document Server

    Tonry, John L

    2010-01-01

    Earth is bombarded by meteors, occasionally by one large enough to cause a significant explosion and possible loss of life. Although the odds of a deadly asteroid strike in the next century are low, the most likely impact is by a relatively small asteroid, and we suggest that the best mitigation strategy in the near term is simply to move people out of the way. We describe an "early warning" system that could provide a week's notice of most sizable asteroids or comets on track to hit the Earth. This system, dubbed "Asteroid Terrestrial-impact Last Alert System" (ATLAS), comprises two observatories separated by about 100km that simultaneously scan the visible sky twice a night, and can be implemented immediately for relatively low cost. The sensitivity of ATLAS permits detection of 140m asteroids (100 Mton impact energy) three weeks before impact, and 50m asteroids a week before arrival. An ATLAS alarm, augmented by other observations, should result in a determination of impact location and time that is accura...

  4. An ISU study of asteroid mining

    Science.gov (United States)

    Burke, J. D.

    During the 1990 summer session of the International Space University, 59 graduate students from 16 countries carried out a design project on using the resources of near-earth asteroids. The results of the project, whose full report is now available from ISU, are summarized. The student team included people in these fields: architecture, business and management, engineering, life sciences, physical sciences, policy and law, resources and manufacturing, and satellite applications. They designed a project for transporting equipment and personnel to a near-earth asteroid, setting up a mining base there, and hauling products back for use in cislunar space. In addition, they outlined the needed precursor steps, beginning with expansion of present ground-based programs for finding and characterizing near-earth asteroids and continuing with automated flight missions to candidate bodies. (To limit the summer project's scope the actual design of these flight-mission precursors was excluded.) The main conclusions were that asteroid mining may provide an important complement to the future use of lunar resources, with the potential to provide large amounts of water and carbonaceous materials for use off earth. However, the recovery of such materials from presently known asteroids did not show an economic gain under the study assumptions; therefore, asteroid mining cannot yet be considered a prospective business.

  5. Asteroid Models from Multiple Data Sources

    CERN Document Server

    Durech, J; Delbo, M; Kaasalainen, M; Viikinkoski, M

    2015-01-01

    In the past decade, hundreds of asteroid shape models have been derived using the lightcurve inversion method. At the same time, a new framework of 3-D shape modeling based on the combined analysis of widely different data sources such as optical lightcurves, disk-resolved images, stellar occultation timings, mid-infrared thermal radiometry, optical interferometry, and radar delay-Doppler data, has been developed. This multi-data approach allows the determination of most of the physical and surface properties of asteroids in a single, coherent inversion, with spectacular results. We review the main results of asteroid lightcurve inversion and also recent advances in multi-data modeling. We show that models based on remote sensing data were confirmed by spacecraft encounters with asteroids, and we discuss how the multiplication of highly detailed 3-D models will help to refine our general knowledge of the asteroid population. The physical and surface properties of asteroids, i.e., their spin, 3-D shape, densit...

  6. Asteroid secular dynamics: Ceres' fingerprint identified

    CERN Document Server

    Novaković, Bojan; Tsirvoulis, Georgios; Knezević, Zoran

    2015-01-01

    Here we report on the significant role of a so far overlooked dynamical aspect, namely a secular resonance between the dwarf planet Ceres and other asteroids. We demonstrate that this type of secular resonance can be the dominant dynamical factor in certain regions of the main asteroid belt. Specifically, we performed a dynamical analysis of the asteroids belonging to the (1726) Hoffmeister family. To identify which dynamical mechanisms are actually at work in this part of the main asteroid belt, i.e. to isolate the main perturber(s), we study the evolution of this family in time. The study is accomplished using numerical integrations of test particles performed within different dynamical models. The obtained results reveal that the post-impact evolution of the Hoffmeister asteroid family is a direct consequence of the nodal secular resonance with Ceres. This leads us to the conclusion that similar effects must exist in other parts of the asteroid belt. In this respect, the obtained results shed light on an i...

  7. Lightcurves of the Karin family asteroids

    Science.gov (United States)

    Yoshida, Fumi; Ito, Takashi; Dermawan, Budi; Nakamura, Tsuko; Takahashi, Shigeru; Ibrahimov, Mansur A.; Malhotra, Renu; Ip, Wing-Huen; Chen, Wen-Ping; Sawabe, Yu; Haji, Masashige; Saito, Ryoko; Hirai, Masanori

    2016-05-01

    The Karin family is a young asteroid family formed by an asteroid breakup 5.8 Myr ago. Since the members of this family probably have not experienced significant orbital or collisional evolution yet, it is possible that they still preserve properties of the original family-forming event in terms of their spin state. We carried out a series of photometric observations of the Karin family asteroids, and here we report on the analysis of the lightcurves including the rotation period of eleven members. The mean rotation rate of the Karin family members turned out to be much lower than those of near-Earth asteroids or small main belt asteroids (diameter D 130 km). We investigated a correlation between the peak-to-trough variation and the rotation period of the eleven Karin family asteroids, and found a possible trend that elongated members have lower spin rates, and less elongated members have higher spin rates. However, this trend has to be confirmed by another series of future observations.

  8. Digging in one last time for the LHC

    CERN Multimedia

    2003-01-01

    A landmark event occurred during the second week of March, when the final cubic metres of earth were cleared away, completing the excavation phase for the entire LHC project . The event took place at Point 5, where the CMS detector will be installed, as civil engineering teams finished digging the cavern that connects the LHC tunnel with the bypass tunnel around the experimental cavern. Two new access shafts, two large caverns, two ancillary caverns, as well as the connecting tunnels have been excavated by the civil engineering teams. "The engineers heaved a huge sigh of relief when the work was done, because the excavations were quite risky. Anything can happen, and the risk of delays was far from zero," explains Jean Luc Baldy Head of ST Division's civil engineering group. This was especially true around Point 5, where unusual geology created some problems. The moraine-molasse interface lies 50 metres beneath the surface, or just about 18 metres above the roof of the caverns. Because the moraine consists of...

  9. Tunnel digging machine digging anchor support application integration technology%机掘巷道掘锚支一体化技术的应用

    Institute of Scientific and Technical Information of China (English)

    刘勋; 李善飞; 曹淑良

    2014-01-01

    掘进、支护、运输不能平行作业成为制约机掘巷道单进水平提升的瓶颈,翟镇煤矿自主研发连体自移超前支架与综掘机配套施工,实现掘进→无支护→临时超前支护→永久性支护的连掘连支衔接过渡,实现真正意义上掘锚支平行作业一体化。%The excavation, shoring, parallel operation of transport can not become a constraint machines digging into the roadway to enhance the level of a single bottleneck Zhaizhen Coal piece from moving ahead independently developed digging Machine supporting bracket and construction, to achieve tunneling → No supporting → temporary forepoling →permanent support convergence even dig even support the transition, dig anchor support parallel operations to achieve integration in the true sense.

  10. Lightcurves for Two Near-Earth Asteroids by Asteroids Observers (OBAS) - MPPD: 2016 April-May

    Science.gov (United States)

    Martinez, Vicente Mas; Silva, Gonzalo Fornas; Martinez, Angel Flores; Garceran, Alfonso Carreno; Mansego, Enrique Arce; Rodriguez, Pedro Brines; de Haro, Juan Lozano; Silva, Alvaro Fornas; Chiner, Onofre Rodrigo; Porta, David Herrero

    2016-10-01

    We report on the results of photometric analysis of two near-Earth asteroids (NEA) by Asteroids Observers (OBAS). This work is part of the Minor Planet Photometric Database (MPPD) project initiated by a group of Spanish amateur astronomers. We have managed to obtain a number of accurate and complete lightcurves as well as some additional incomplete lightcurves to help analysis at future oppositions.

  11. Eighteen Asteroids Lightcurves at Asteroides Observers (OBAS) - MPPD: 2016 March-May

    Science.gov (United States)

    Mansego, Enrique Arce; Rodriguez, Pedro Brines; de Haro, Juan Lozano; Chiner, Onofre Rodrigo; Silva, Alvaro Fornas; Porta, David Herrero; Martinez, Vicente Mas; Silva, Gonzalo Fornas; Garceran, Alfonso Carreno

    2016-10-01

    We report on the analysis of photometric observations of 18 main-belt asteroids (MBA) done by Asteroides Observers (OBAS). This work is part of the Minor Planet Photometric Database program initiated by a group of Spanish amateur astronomers. We have managed to obtain a number of accurate and complete lightcurves as well as some additional incomplete lightcurves to help analysis at future oppositions.

  12. Twenty-three Asteroids Lightcurves at Observadores de Asteroides (OBAS): 2015 October - December

    Science.gov (United States)

    Aznar Macias, Amadeo; Carreno Garcerain, Alfonso; Arce Mansego, Enrique; Brines Rodriguez, Pedro; Lozano de Haro, Juan; Fornas Silva, Alvaro; Fornas Silva, Gonzalo; Mas Martinez, Vicente; Rodrigo Chiner, Onofre

    2016-04-01

    We report on the photometric analysis results for 23 main-belt asteroids (MBA) done by Observadores de Asteroides (OBAS). This work is part of the Minor Planet Photometric Database that was initiated by a group of Spanish amateur astronomers. We have managed to obtain a number of accurate, complete lightcurves as well as some additional incomplete lightcurves to help analysis at future oppositions.

  13. Lightcurve Survey of V-type Asteroids in the Inner Asteroid Belt

    CERN Document Server

    Hasegawa, Sunao; Mito, Hiroyuki; Sarugaku, Yuki; Ozawa, Tomohiko; Kuroda, Daisuke; Nishihara, Setsuko; Harada, Akari; Yoshida, Michitoshi; Yanagisawa, Kenshi; Shimizu, Yasuhiro; Nagayama, Shogo; Toda, Hiroyuki; Okita, Kouji; Kawai, Nobuyuki; Mori, Machiko; Sekiguchi, Tomohiko; Ishiguro, Masateru; Abe, Takumi; Abe, Masanao

    2013-01-01

    We have observed the lightcurves of 13 V-type asteroids ((1933) Tinchen, (2011) Veteraniya, (2508) Alupka, (3657) Ermolova, (3900) Knezevic, (4005) Dyagilev, (4383) Suruga, (4434) Nikulin, (4796) Lewis, (6331) 1992 $\\mathrm{FZ_{1}}$, (8645) 1998 TN, (10285) Renemichelsen, and (10320) Reiland). Using these observations we determined the rotational rates of the asteroids, with the exception of Nikulin and Renemichelsen. The distribution of rotational rates of 59 V-type asteroids in the inner main belt, including 29 members of the Vesta family that are regarded as ejecta from the asteroid (4) Vesta, is inconsistent with the best-fit Maxwellian distribution. This inconsistency may be due to the effect of thermal radiation Yarkovsky--O'Keefe--Radzievskii--Paddack (YORP) torques, and implies that the collision event that formed V-type asteroids is sub-billion to several billion years in age.

  14. 挖拔式木薯收获机的研制与样机试验%Development and prototype trial of digging-pulling style cassava harvester

    Institute of Scientific and Technical Information of China (English)

    廖宇兰; 孙佑攀; 刘世豪; 陈丹萍; 王高平

    2012-01-01

    Aim at the complexity of cassava tuber distributing in the soil,in order to harvest cassava tuber from different soils with a variety of hard levels,referencing the basic principles and structure of potatoes,garlic,sweet potatoes and other root crops harvesting machinery,a kind of digging-pulling style cassava harvester was developed based on cassava's biological and physical characteristics,which can complete tuber's digging,transportation,separation and other work simultaneously.The digging shovel,clamping conveyor and power transmission mechanism were designed and the key parameters were determined.The key parameters of the grizzly bar-type shovel is shovel's plane angle of on more 20°,the shovel's length of is 550 mm and shovel's width is 1000 mm.The total transmission ratio is 2.29,gearbox's transmission ratio is 2.The gearbox output shaft speed is 500 r/min.The chain transmission ratio is 1.15,and output speed is 435 r/min.The digging-pulling cassava harvester should be used with medium-sized tractor.Through the trial of the prototype and field test,the results showed that digging-pulling cassava harvester runs smoothly,and reaches the combination of digging and pulling to harvest cassava.%针对木薯块根在土壤中分布的复杂性,为了将木薯块根顺利地从各种松硬程度不同的土壤收获出来,模拟人工收获木薯的机理,借鉴马铃薯、大蒜、红薯等根茎类作物收获机械的基本原理和结构,以木薯生物和物理特性为依据,该文研制出一种可一次性完成薯块的挖掘、分离、输送等工作的挖拔式木薯收获机.该文主要介绍了挖掘铲、夹持输送机构及动力传输机构及关键参数的确定.该栅条式挖掘铲的关键参数为铲平面倾角为20°,铲长为550 mm,铲宽为1 000 mm.计算出整机总传动比为2.29,变速箱传动比为2,输出速度为500 r/min,链传动的传动比为1.15,输出速度为435 r/min.该机与中型拖拉机配套使用,通过样机的

  15. Using Dust from Asteroids as Regolith Microsamples

    Science.gov (United States)

    Cohen, B. A.; Klima, Rachel; Chabot, N. L.; Rivkin, A. S.

    2015-01-01

    Meteorite science is rich with compositional indicators by which we classify parent bodies, but few sample groups are definitively linked with asteroid spectra. More robust links need to be forged between meteorites and their parent bodies to understand the composition, diversity and distribution. A major link can be sample analysis of the parent body material and comparison with meteorite data. Hayabusa, the first sample return mission of the Japanese Aerospace Exploration Agency (JAXA), was developed to rendezvous with and collect samples from asteroid Itokawa and return them to Earth. Thousands of sub-100 micron particles were recovered, apparently introduced during the spacecraft impact into the surface of the asteroid, linking the asteroid Itokawa to LL chondrites [1]. Upcoming missions Hayabusa 2 and OSIRIS-REx will collect more significant sample masses from asteroids. In all these cases, the samples are or will be a collection of regolith particles. Sample return to earth is not the only method for regolith particle analysis. Dust is present around all airless bodies, generated by micrometeorite impact into their airless surfaces, which in turn lofts regolith particles into a "cloud" around the body. The composition, flux, and size-frequency distribution of dust particles can provide significant insight into the geological evolution of airless bodies [2]. For example, the Cassini Cosmic Dust Analyzer (CDA) detected salts in Enceladus' icy plume material, providing evidence for a subsurface ocean in contact with a silicate seafloor [3]. Similar instruments have flown on the Rosetta, LADEE, and Stardust missions. Such an instrument may be of great use in obtaining the elemental, isotopic and mineralogical composition measurement of dust particles originating from asteroids without returning the samples to terrestrial laboratories. We investigated the ability of a limited sample analysis capability using a dust instrument to forge links between asteroid

  16. Aqueous alteration on main-belt asteroids

    Science.gov (United States)

    Fornasier, S.; Lantz, C.; Barucci, M.; Lazzarin, M.

    2014-07-01

    The study of aqueous alteration is particularly important for unraveling the processes occurring during the earliest times in Solar System history, as it can give information both on the thermal processes and on the localization of water sources in the asteroid belt, and for the associated astrobiological implications. The aqueous alteration process produces the low temperature (< 320 K) chemical alteration of materials by liquid water which acts as a solvent and produces materials like phyllosilicates, sulphates, oxides, carbonates, and hydroxides. This means that liquid water was present in the primordial asteroids, produced by the melting of water ice by heating sources, very probably by ^{26}Al decay. Hydrated minerals have been found mainly on Mars surface, on primitive main-belt asteroids (C, G, B, F, and P-type, following the classification scheme by Tholen, 1984) and possibly also on few transneptunian objects. Reflectance spectroscopy of aqueous altered asteroids shows absorption features in the 0.6-0.9 and 2.5-3.5-micron regions, which are diagnostic of, or associated with, hydrated minerals. In this work, we investigate the aqueous alteration process on a large sample of 600 visible spectra of C-complex asteroids available in the literature. We analyzed all these spectra in a similar way to characterize the absorption-band parameters (band center, depth, and width) and spectral slope, and to look for possible correlations between the aqueous alteration process and the asteroids taxonomic classes, orbital elements, heliocentric distances, albedo, and sizes. We find that 4.6 % of P, 7.7 % of F, 9.8 % of B, 50.5 % of C, and 100 % of the G-type asteroids have absorption bands in the visible region due to hydrated silicates. Our analysis shows that the aqueous alteration sequence starts from the P-type objects, practically unaltered, and increases through the P → F → B → C → G asteroids, these last being widely aqueously altered, strengthening thus

  17. Near-Earth Asteroid Scout

    Science.gov (United States)

    McNutt, Leslie; Johnson, Les; Clardy, Dennon; Castillo-Rogez, Julie; Frick, Andreas; Jones, Laura

    2014-01-01

    Near-Earth Asteroids (NEAs) are an easily accessible object in Earth's vicinity. Detections of NEAs are expected to grow in the near future, offering increasing target opportunities. As NASA continues to refine its plans to possibly explore these small worlds with human explorers, initial reconnaissance with comparatively inexpensive robotic precursors is necessary. Obtaining and analyzing relevant data about these bodies via robotic precursors before committing a crew to visit a NEA will significantly minimize crew and mission risk, as well as maximize exploration return potential. The Marshall Space Flight Center (MSFC) and Jet Propulsion Laboratory (JPL) are jointly examining a mission concept, tentatively called 'NEA Scout,' utilizing a low-cost CubeSats platform in response to the current needs for affordable missions with exploration science value. The NEA Scout mission concept would be a secondary payload on the Space Launch System (SLS) Exploration Mission 1 (EM-1), the first planned flight of the SLS and the second un-crewed test flight of the Orion Multi-Purpose Crew Vehicle (MPCV).

  18. SOFIA observations of dark asteroids: Evidence for hydrated minerals on asteroidal surfaces?

    Science.gov (United States)

    McAdam, Margaret; Sunshine, Jessica M.; Kelley, Michael S. P. T.

    2015-11-01

    We present results from recent SOFIA+FORCAST observations of three primitive asteroids and compare these to archived Spitzer Space Telescope (Spitzer) observations of similar objects. Three asteroids from a total of 12 have been observed with SOFIA+FORCAST in our Cycle-3 campaign. Currently, we have observed asteroids 38 Leda, 194 Prokne with both G111 and G227 grisms and asteroid 266 Aline with G227. Both wavelength regions (G111: 8.5-13.5-μm and G227: 17.6-27.7) have recently been shown to contain spectral features directly related degree of alteration of primitive meteorites, including unaltered CO and CV meteorites (McAdam, et al., 2015a ,b). Spectral features in the 17.6-27.7-μm region can be indicative of olivine (19.5-μm), hydrated minerals (21-μm) and silica glass (22-μm). Spitzer observed eight large, primitive, main-belt asteroids using both low-resolution modes (short-low, SL and long-low, LL) of the Infrared Spectrograph (IRS) covering 8.5-38-μm. Additionally, Spitzer observed 22 dark primitive asteroids in the 8.5-13.5-μm region. Asteroids observed with Spitzer fall into three categories: asteroids with a 12-μm feature of 1-5% depth, interpreted as ~60-70% hydrated minerals (McAdam, et al., 2015a) asteroids with a broader 12-13-μm feature with strengths ranging from 4-6% with potential features between 19-22-μm (where observed) and asteroids with a strong 13-μm feature (5-10%), 15-μm and potentially 19-22-μm features (where observed) interpreted as olivine-rich. However, the uncertain calibration at the edges of the LL spectral orders complicates feature identification. 194 Prokne has a feature ~12-13-μm feature and potentially a broad feature between 20-22-μm. This is consistent with primitive asteroids observed with Spitzer that are interpreted as hydrated mineral-bearing. 38 Leda is largely featureless at the noise limit of the spectrum with a potential feature at 25-μm, unlike asteroids observed by Spitzer. 266 Aline has a weak

  19. 78 FR 64253 - NASA Asteroid Initiative Idea Synthesis Workshop

    Science.gov (United States)

    2013-10-28

    ... SPACE ADMINISTRATION NASA Asteroid Initiative Idea Synthesis Workshop AGENCY: National Aeronautics and Space Administration. ACTION: Notice of Continuation of public conference to examine ideas in response... Administration announces that the agency will resume the NASA Asteroid Initiative Idea Synthesis...

  20. CCD-Photometry and Pole Coordinates for Eight Asteroids

    Science.gov (United States)

    Shevchenko, V. G.; Tungalag, N.; Chiorny, V. G.; Gaftonyuk, N. M.; Krugly, Y. N.; Harris, A. W.; Young, J. W.

    2012-05-01

    The long time photometric observations were carried out for eight asteroids: (122) Gerda, (153) Hilda, (190) Ismene, (221) Eos, (411) Xanthe, (679) Pax, (700) Auravictrix, (787) Moskva. For the observed asteroids were determined new pole coordinates.

  1. A Fast Ellipsoid Model for Asteroids Inverted From Lightcurves

    CERN Document Server

    Lu, Xiaoping; You, Zhong

    2012-01-01

    The research about asteroids attracts more and more attention recently, especially focusing on their physical structures, such as the spin axis, the rotation period and the shape. The long distance between Earth observers and asteroids makes it impossible to get the shape and other parameters of asteroids directly with the exception of the NEAs (Near Earth Asteroids) and others passed by some spacecrafts. Generally photometric measurement is still the main way to obtain the research data for asteroids now, i.e. the lightcurves recording the brightness and positions of asteroids. Supposing that the shape of the asteroid is a triaxial ellipsoid with a stable spinning status, a new method is present in this article to reconstruct the shape models of asteroids from the lightcurves, with the other physical parameters together. By applying a special curvature function, the method calculates the brightness integration on a unit sphere and Lebedev Quadrature is employed for the discretization. At last the method sear...

  2. Asteroid rotation rates depend on diameter and type

    Energy Technology Data Exchange (ETDEWEB)

    Dermott, S.F.; Murray, C.D. (Cornell Univ., Ithaca, NY (USA). Center for Radiophysics and Space Research)

    1982-04-01

    The rotational frequency of main-belt asteroids is shown here to depend on both asteroidal type and diameter. If asteroids of any one diameter are considered then, on average, M asteroids rotate faster than S asteroids which in turn rotate faster than C asteroids. This shows that asteroids which have been classified by their surface properties alone have different bulk properties. For all three types, although the dispersions of the frequencies are large, it is proved that the mean frequency increases linearly with the mean diameter. In both the C and S plots of mean rotational frequency against mean diameter there are discontinuities at diameters approximately equal to 125 km and approximately equal to 105 km, respectively, which may differentiate primordial asteroids from their collisional products.

  3. A Search for Asteroids, Moons, and Rings Orbiting White Dwarfs

    CERN Document Server

    Di Stefano, Rosanne; Kawaler, Steven D

    2009-01-01

    Do white dwarfs host asteroid systems? Although several lines of argument suggest that white dwarfs may be orbited by large populations of asteroids, transits would provide the most direct evidence. We demonstrate that the Kepler mission has the capability to detect transits of white dwarfs by asteroids. Because white-dwarf asteroid systems, if they exist, are likely to contain many asteroids orbiting in a spatially extended distribution, discoveries of asteroid transits can be made by monitoring only a small number of white dwarfs, compatible with Kepler's primary mission, which is to monitor stars with potentially habitable planets. Possible future missions that survey ten times as many stars with similar sensitivity and minute-cadence monitoring can establish the characteristics of asteroid systems around white dwarfs, such as the distribution of asteroid sizes and semimajor axes. Transits by planets would be more dramatic, but the probability that they will occur is lower. Ensembles of planetary moons and...

  4. Brazil Nuts on Eros: Size-Sorting of Asteroid Regolith

    Science.gov (United States)

    Asphaug, E.; King, P. J.; Swift, M. R.; Merrifield, M. R.

    2001-01-01

    We consider the hypothesis that frequent cratering produces size- or compositionally-sorted asteroid regolith, affecting the structure, texture, and in extreme cases the shape of asteroids. Additional information is contained in the original extended abstract.

  5. Human Robotic Systems (HRS): Robotic Technologies for Asteroid Missions Element

    Data.gov (United States)

    National Aeronautics and Space Administration — During 2014, the Robotic Technologies for Asteroid Missions activity has four tasks:Asteroid Retrieval Capture Mechanism Development and Testbed;Mission Operations...

  6. Philosophy and updating of the asteroid photometric catalogue

    Science.gov (United States)

    Magnusson, Per; Barucci, M. Antonietta; Capria, M. T.; Dahlgren, Mats; Fulchignoni, Marcello; Lagerkvist, C. I.

    1992-01-01

    The Asteroid Photometric Catalogue now contains photometric lightcurves for 584 asteroids. We discuss some of the guiding principles behind it. This concerns both observers who offer input to it and users of the product.

  7. The Strength of Rubble Pile Asteroids

    Science.gov (United States)

    Scheeres, D. J.; Sanchez, P.

    2012-12-01

    The rubble pile hypothesis for small asteroids in the Near Earth and Main Belt populations have been driven by several factors, including the observed high porosity of those bodies whose mass have been measured, the evident limitation on spin rate of asteroids larger than ~500 meters, and direct observation of the surface morphology of these bodies. Given these observations, it has been presumed that small asteroids should evolve as if they were cohesionless collections of grains. Detailed geophysical analysis of these bodies by Holsapple (Icarus 2010) show that cohesionless bodies will evolve under the addition of angular momentum by the YORP effect into more distended and, paradoxically, more slowly rotating bodies. Additional analysis in Holsapple (Icarus 2007) has shown that cohesional strength within a rubble pile could strengthen a collection of grains to the point where they could sustain rapid rotation. In our current talk we use the above as a starting point and incorporate new observations of the asteroid morphology driven by recent analysis of asteroid Itokawa by the Hayabusa science team and research on the mechanics of grains in the space environment (Scheeres et al. 2010). Analysis of images of Itokawa determined a measured size distribution of 1/d^3 for larger grains on asteroid Itokawa (Michikami et al., Earth Planets Space, 60, 13-20, 2008). Analysis of the sample shows the presence of micron sized dust on that asteroid's surface (Tsuchiyama et al., Science 333, 1125, 2011). Combining these observations provides a global indication of grain distribution within rubble piles. Even assuming a less steep distribution of 1/d^2 for dust grains smaller than 1 mm in size, the interior of Itokawa should still be dominated by the finest dust grains, with the mean grain size equal to ~ twice the smallest grain in the distribution. One implication of this result is that fines are present on the surface of the rubble pile Itokawa and thus should be distributed

  8. Thermal Tomography of Asteroid Surface Structure

    CERN Document Server

    Harris, Alan

    2016-01-01

    Knowledge of the surface thermal inertia of an asteroid can provide insight into surface structure: porous material has a lower thermal inertia than rock. We develop a means to estimate thermal inertia values of asteroids and use it to show that thermal inertia appears to increase with spin period in the case of main-belt asteroids (MBAs). Similar behavior is found on the basis of thermophysical modeling for near-Earth objects (NEOs). We interpret our results in terms of rapidly increasing material density and thermal conductivity with depth, and provide evidence that thermal inertia increases by factors of 10 (MBAs) to 20 (NEOs) within a depth of just 10 cm. Our results are consistent with a very general picture of rapidly changing material properties in the topmost regolith layers of asteroids and have important implications for calculations of the Yarkovsky effect, including its perturbation of the orbits of potentially hazardous objects and those of asteroid family members after the break-up event. Eviden...

  9. Detecting Mass Loss in Main Belt Asteroids

    Science.gov (United States)

    Sandberg, Erik; Rajagopal, Jayadev; Ridgway, Susan E.; Kotulla, Ralf C.; Valdes, Francisco; Allen, Lori

    2016-01-01

    Sandberg, E., Rajagopal, J., Ridgway, S.E, Kotulla, R., Valdes, F., Allen, L.The Dark Energy Camera (DECam) on the 4m Blanco telescope at the Cerro Tololo Inter-American Observatory (CTIO) is being used for a survey of Near Earth Objects (NEOs). Here we attempt to identify mass loss in main belt asteroids (MBAs) from these data. A primary motivation is to understand the role that asteroids may play in supplying dust and gas for debris disks. This work focuses on finding methods to automatically pick out asteroids that have qualities indicating possible mass loss. Two methods were chosen: looking for flux above a certain threshold in the asteroid's radial profile, and comparing its PSF to that of a point source. After sifting through 490 asteroids, several have passed these tests and should be followed up with a more rigorous analysis.Sandberg was supported by the NOAO/KPNO Research Experience for Undergraduates (REU) Program which is funded by the National Science Foundation Research Experiences for Undergraduates Program (AST-1262829)

  10. On the Discovery of the Asteroid 3784 Chopin

    Science.gov (United States)

    Elst, E. W.

    Le 31 octobre 1986 lords d'une campagne de recherche d'asteroides a l'observatoire de Haute Provence, un asteroide de septieme magnitude fut decouvert. A l'occasion de l'opposition consecutive en 1988, l'asteroide fut observe a nouveau a l'observatoire de Haute Provence, ce qui entraina la numerotation definitive. L'asteroide recoit le numero 3874 et le nom du grand compositeur polonais, Chopin.

  11. A Fast Ellipsoid Model for Asteroids Inverted From Lightcurves

    OpenAIRE

    Lu, Xiaoping; Zhao, Haibin; You, Zhong

    2012-01-01

    The research about asteroids attracts more and more attention recently, especially focusing on their physical structures, such as the spin axis, the rotation period and the shape. The long distance between Earth observers and asteroids makes it impossible to get the shape and other parameters of asteroids directly with the exception of the NEAs (Near Earth Asteroids) and others passed by some spacecrafts. Generally photometric measurement is still the main way to obtain the research data for ...

  12. Walking softly : using bioremediation to reclaim sites leaves a smaller footprint than traditional dig-and-dump technologies

    International Nuclear Information System (INIS)

    Recent developments in the bioremediation industry in Alberta were outlined. The market for bioremediation services in the United States alone is estimated to hit $1 billion by 2010 and has become a staple of the U.S. Environmental Protection Agency's emergency management practices in the event of an oil spill. Alberta Environment has recently updated its policies and guidance documents on contaminated sites management, and is planning a manual that will include best bioremediation practices. Advances in the science and technology of bioremediation and a rise in environmental awareness have contributed to the sector's growth in recent years. In the past, oil companies in Alberta typically reclaimed sites by digging up contaminated soil and trucking it to landfills. Recent techniques developed by industry and bioremediation experts now mean that soil profiles can remain undisturbed, and biological treatment amendments are often introduced into the fractures to destroy contaminants where they lie. The National Research Council's Biotechnology Research Institute (NRC-BRI) is now conducting research to identify and profile unknown micro-organisms to improve conditions for the breakdown of toxins. Bioremediation techniques are also being used in urban redevelopment. It was concluded that while the environmental industry is regulatory-driven, many oil and mining companies are deciding to invest in remediation instead of waiting until a later date. A list of new bioremediation partnerships with industry, government and municipalities was also provided. 2 figs

  13. Dynamic wind turbine models in power system simulation tool DIgSILENT

    DEFF Research Database (Denmark)

    Hansen, A.D.; Jauch, C.; Sørensen, Poul Ejnar;

    2004-01-01

    The present report describes the dynamic wind turbine models implemented in the power system simulation tool DIgSILENT (Version 12.0). The developed models are a part of the results of a national research project, whose overall objective is to create amodel database in different simulation tools....... The report contains both the description of DIgSILENT built-in models for the electrical components of a grid connected wind turbine (e.g. inductiongenerators, power converters, transformers) and the models developed by the user, in the dynamic simulation language DSL of DIgSILENT, for the non......-electrical components of the wind turbine (wind model, aerodynamic model, mechanical model). Theinitialisation issues on the wind turbine models into the power system simulation are also presented. However, the main attention in this report is drawn to the modelling at the system level of two wind turbine concepts: 1...

  14. File list: InP.Dig.20.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

    Lifescience Database Archive (English)

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  15. File list: InP.Dig.50.AllAg.Intestinal_stem_cells [Chip-atlas[Archive

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