On deuterium generation in the early solar system

Details On deuterium generation in the early solar system On deuterium generation in the early solar system

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1469u&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 469.

Physics

Solar System Evolution, Deuterium, Shock Wave Propagation, Supernova Remnants, Power Spectra, Solar Cosmic Rays, Solar Corona, Energetic Particles, Galactic Cosmic Rays, Gas Giant Planets

Scientific paper

It is suggested that, under the conditions of shock wave propagation in the formation stage of the solar system, not more than about 40 percent of the average abundance of deuterium could be generated. Preliminary contamination of the protosolar nebula through deuterium produced in similar processes in about ten earlier supernova explosions should be assumed.

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