| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 6439284 | Geochimica et Cosmochimica Acta | 2012 | 15 Pages |
Abstract
The 26Al-26Mg systematics of this Leoville Type B CAI suggest it experienced a final melting event at â¼50Â ka after the initial Al-Mg fractionation event. This may correspond to melting during the active protostar stage (known as “Class I”), during which sporadic high temperature heating events repeatedly affected refractory solids in the solar nebula.
Related Topics
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Geochemistry and Petrology
Authors
Noriko T. Kita, Takayuki Ushikubo, Kim B. Knight, Ruslan A. Mendybaev, Andrew M. Davis, Frank M. Richter, John H. Fournelle,