A New Model for the Origin of Type-B CAIs

Details A New Model for the Origin of Type-B CAIs A New Model for the Origin of Type-B CAIs

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1015r&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1015

Physics

Scientific paper

Most CAIs formed near the Sun, but Type-Bs formed in the CV-CK region
after Type-As collided inelastically, incorporated some forsterite-rich
dust, melted and partially evaporated. B3s formed after greater amounts
of forsterite were incorporated.

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