Helium and Neon in Carbon-rich Phases of Interplanetary Dust Particles

Details Helium and Neon in Carbon-rich Phases of Interplanetary Dust Particles Helium and Neon in Carbon-rich Phases of Interplanetary Dust Particles

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.2074p&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.2074

Physics

Scientific paper

IDPs showing evidence of atmospheric entry heating to high temperature
nevertheless retained large amounts of He in highly refractory, probably
carbonaceous sites. Carbon is also a major He and Ne carrier in a
particle not strongly heated on entry.

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