Results 231 to 240 of about 22,696,219 (287)
The late formation of chondrites as a consequence of Jupiter-induced gaps and rings. [PDF]
Sci AdvSrivastava B, Izidoro A.
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Different Scales, Different Rules: How Do Temperature and Radiation Across Macro- and Microclimate Shape Forest Insect Traits? [PDF]
Ecol EvolPickert R +11 more
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Mechanical evolution of small solar system bodies
, 2023 This dissertation presents a series of studies that develop and apply numerical modeling techniques to small bodies in the solar system. We are particularly interested in low-energy deformations, collisions, and disruptions, and our subjectsrange from near-Earth asteroids to Kuiper belt contact binaries in the farthest reaches of the solar system.
Marohnic, Julian Charles
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Small Solar System Bodies as granular media [PDF]
Astronomy and Astrophysics Review, 2019 Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the ...
Derek C Richardson +2 more
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2002
Number of minor planets having well-determined orbits, cataloged by permanent designations (numbers) as of 1998, January 1: 8125. Number of known minor planets having less well-determined orbits, cataloged by provisional designations: > 25, 000. Most are located in the Main-belt, between Mars and Jupiter. Semimajor axis, range 2.06 to 3.28 AU, mean a =
Richard P. Binzel +2 more
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Number of minor planets having well-determined orbits, cataloged by permanent designations (numbers) as of 1998, January 1: 8125. Number of known minor planets having less well-determined orbits, cataloged by provisional designations: > 25, 000. Most are located in the Main-belt, between Mars and Jupiter. Semimajor axis, range 2.06 to 3.28 AU, mean a =
Richard P. Binzel +2 more
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Migration of Small Bodies in the Solar System
Earth, Moon, and Planets, 1996We investigate several parts of the process of migration of small bodies to the Earth from the asteroid and transneptunian belts. The obtained characteristic times up to collisions of near-Earth objects with the Earth are less than those obtained by other scientists.
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Small Bodies of the Solar System
International Astronomical Union Colloquium, 1984Schmidt telescopes are ideal for many types of survey work, and this includes surveying the solar system. Schmidt cameras have the advantages of speed and wide fields for rapid coverage of large areas of the sky, and good image quality over the entire field. The small focal ratios also have the effect of enhancing low surface-brightness features.
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Regoliths on Small Bodies in the Solar System
Annual Review of Earth and Planetary Sciences, 1982A regolith is defined as a layer or mantle of loose, incoherent, rocky material of whatever origin, that nearly everywhere forms the surface of the land and rests on coherent bedrock. The regoliths on many planetary bodies are the result of continual impacts, which transform coherent surfaces into fragmental debris.
K R Housen, L L Wilkening
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