Presolar Graphite from Murchison

Details Presolar Graphite from Murchison Presolar Graphite from Murchison

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1098a&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1098

Physics

Scientific paper

We have analyzed 1642 graphite grains from four Murchison fractions.
Many grains in lower-density fractions KE3 and KFA1 originated from
supernovae. A significant number of grains in higher-density fractions
KFB1 and KFC1 formed in low-metallicity AGB stars.

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