Reevaluation of the 53Mn-53Cr Systematic in the Basaltic Achondrites

Details Reevaluation of the 53Mn-53Cr Systematic in the Basaltic Achondrites Reevaluation of the 53Mn-53Cr Systematic in the Basaltic Achondrites

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1946t&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1946

Physics

1

Scientific paper

The 53Mn-53Cr isotopic evolution of basaltic achondrites is reevaluated.
The initial 53Cr/52Cr is lower than previously thought. It follows that
the source of the HED meteorites is volatile depleted with lower than
solar Mn/Cr ratio.

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