Gas-rich meteorites - Probes for particle environment and dynamical processes in the inner solar system

Details Gas-rich meteorites - Probes for particle environment and dynamical processes in the inner solar system Gas-rich meteorites - Probes for particle environment and dynamical processes in the inner solar system

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ssrv...37..111g&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 37, Jan.-Feb. 1984, p. 111-159.

Computer Science

23

Cosmology, Gas Composition, Meteoritic Composition, Solar System, Abundance, Asteroids, Carbonaceous Chondrites, Cometary Atmospheres, Cosmic Rays, Galactic Radiation, Petrography, Radiation Effects, Solar Flares, Solar Wind, Meteorites, Gases, Enrichment, Particles, Dynamics, Energy, Spectra, Solar System, Review, Samples, Meteorite, Abundance, Patterns, Comets, Solar Wind, Asteroids, Isotopes, Composition, Solar Flares, History, Impacts, Interplanetary Dust, Grains, Petrography, Chemistry, Evolution, Ordi

Scientific paper

Although the asteroids are the most plausible candidates for the parent bodies of gas-rich meteorites, dynamical theories have been adduced which favor a cometary origin in certain cases, and some recent studies have indicated that, in the case of gas-rich carbonaceous chondrites, the solar flare irradiation of grains may have occurred prior to the formation of parent bodies. Attention is presently given to advances that have been made in the multidisciplinary studies, encompassing petrography, chemistry, and radiation effects, of the gas-rich meteorites. An evaluation is undertaken of the present understanding of gas-rich meteorite origin and evolution.

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