Initial 26Al Abundance in a Type B CAI: Remelting of Pre-Existing Refractory Solid

Details Initial 26Al Abundance in a Type B CAI: Remelting of Pre-Existing Refractory Solid Initial 26Al Abundance in a Type B CAI: Remelting of Pre-Existing Refractory Solid

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2154k&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2154

Physics

3

Scientific paper

High precision SIMS internal isochron of Leoville 3535-1 type B1 CAI
indicates that it melted 30-40 k.y. after the formation of first
solids in the solar system from refractory precursor solids and possibly
it melted multiple times.

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