Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
6438393 | Geochimica et Cosmochimica Acta | 2014 | 63 Pages |
Abstract
The presence of CM material is an important parameter for understanding the evolution of Vesta's surface. While we have uncovered three further regolithic howardites (â¼13 regolithic total, of â¼41 analysed), further noble gas analysis of HED meteorites is needed to not only determine regolithic origins, but to better characterise the abundance of carbonaceous chondrite material and its effect on the noble gas signatures of such samples.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geochemistry and Petrology
Authors
J.A. Cartwright, U. Ott, D.W. Mittlefehldt,