Dark Mantles Around CM Chondrules are not Accretionary Rims

Details Dark Mantles Around CM Chondrules are not Accretionary Rims Dark Mantles Around CM Chondrules are not Accretionary Rims

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2314w&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2314

Computer Science

1

Scientific paper

Fine dark mantles around some CM chondrules consist of nebular materials
but porosities are low, inconsistent with nebular formation. We suggest
that the mantles resulted from asteroidal impact compaction that
predated aqueous alteration.

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