| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8911067 | Geochimica et Cosmochimica Acta | 2017 | 59 Pages |
Abstract
To summarize, the weight of the evidence favors the conclusion that IIE meteorites were formed by one or more impacts on an HH asteroid. The target probably had a composition like the chondritic materials in Netschaevo, but was unequilibrated and had much higher porosity.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geochemistry and Petrology
Authors
John T. Wasson,