Computer Science
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978metic..13..291h&link_type=abstract
Meteoritics, vol. 13, Sept. 30, 1978, p. 291-303.
Computer Science
1
Carbonaceous Chondrites, Chondrites, Meteoritic Composition, Planetary Evolution, Rare Gases, Solar Wind, Amor Asteroid, Apollo Asteroids, Comets, Orgueil Meteorite, Solar Orbits, Cosmic Rays, Exposure Ages, Chondrites, Meteorites, Origin, Asteroids, Gases, Sun, Ions, Earth, Apollo Asteroids, Amor Asteroids, Carbonaceous Chondrites, C1 Chondrites, Rocks, Regolith, Solar Wind, Comets, Artificial Impacts, Orbits, Flux, Encke, Comet, Cosmic Dust, Formation Of
Scientific paper
Evidence suggesting that chondritic meteorites broke off from parent bodies in earth-crossing orbits is considered. It is suggested that ordinary chondrites have an asteroidal origin, and the possibility that C1 chondrites have a cometary origin is examined. Indications of heavy shock and reheating among L and H chondrites provides support for an asteroidal origin, while the Apollo and Amor objects are too small to be unfragmented asteroids, as proposed in the Anders theory of the origin of gas-rich meteorites. Events associated with the megaregolith are discussed in the framework of the proposed cometary origin of C1 chondrites.
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