Helium, Neon, and Argon in Canyon Diablo Spheroids

Details Helium, Neon, and Argon in Canyon Diablo Spheroids Helium, Neon, and Argon in Canyon Diablo Spheroids

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1720l&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1720

Physics

1

Scientific paper

Despite having melted when they formed, many Canyon Diablo spheroids
retain cosmogenic 38Ar. The concentrations imply that the spheroids'
precursor material mostly came from a shell ~1 m thick centered at a
depth of ~1.2 m in the impactor.

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