Primordially Trapped Heavy Noble Gases in Rumuruti Chondrites?

Details Primordially Trapped Heavy Noble Gases in Rumuruti Chondrites? Primordially Trapped Heavy Noble Gases in Rumuruti Chondrites?

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2793b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2793

Physics

Scientific paper

We discuss Kr and Xe abundances in Rumuruti chondrites. None of the
samples need to contain phase Q gases to explain the results. Phase Q
might have been destroyed by parent body oxidation or by oxidation of
the precursor material in the nebula.

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