Computer Science
Scientific paper
Oct 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ucsd.rept.....m&link_type=abstract
Technical Report, NASA/CR-97-205736; NAS 1.26:205736; UCSD-95-6767R Dept. of Chemistry and Biochemistry
Computer Science
Solar System, Nebulae, Solar System Evolution, Mars Atmosphere, Meteoritic Composition, Cosmic Rays, Nitrogen, Abundance, Spallation, Meteorites, Xenon, Fragmentation, Helium, Isotopes, Signatures, Atmospheric Composition
Scientific paper
The objective of this research is an improved understanding of the early solar system environment and of the processes involved in the nebula and in the evolution of solid bodies. We present results of our studies on the isotopic signatures in selected primitive solar system objects and on the evaluation of the cosmic ray records and of inferred collisional events. Furthermore, we report data of trapped martian atmospheric gases in meteorites and the inferred early evolution of Mars' atmosphere.
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