Predicted Abundances of Cosmogenic Noble Gases in Interplanetary Dust Particles from Different Parent Objects

Details Predicted Abundances of Cosmogenic Noble Gases in Interplanetary Dust Particles from Different Parent Objects Predicted Abundances of Cosmogenic Noble Gases in Interplanetary Dust Particles from Different Parent Objects

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2376k&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

A numerical model is developed to test the idea that interplanetary dust
particles from different parent objects can be distinguished based on
the abundances of cosmogenic noble gases accumulated during transit from
the parent object to the Earth.

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