| Abstract: | CARBONACEOUS chondrites, although comprising only about 2% of known meteorites, are extremely interesting for scientific investigation. Their mineral constitution, and the correspondence between their bulk chemical composition and the solar abundance of condensable elements, indicate that minimum chemical fractionation and thermal alteration have occurred. The mineral phases observed in these primitive chondrites are sufficiently unique, with respect to other meteorite classes, to have elicited considerable speculation about the physical environment in which they formed1-7. ?? 1975 Nature Publishing Group. |
| Genre: | Article |
| ProdID: | 70001240 |
| Citation Author: | Herndon, J. M.; Rowe, M. W.; Larson, E. E.; Watson, D. E. |
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| Citation End Page: | 518 |
| Citation Issue: | 5492 |
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| Citation Language: | English |
| Citation Larger Work Title: | Nature |
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| Citation Search Results Text: | Origin of magnetite and pyrrhotite in carbonaceous chondrites; 1975; Article; Journal; Nature; Herndon, J. M.; Rowe, M. W.; Larson, E. E.; Watson, D. E. |
| Citation Start Page: | 516 |
| Citation Volume: | 253 |
| Citation Year: | 1975 |
| Type: | citation/reference |
| Text: | Origin of magnetite and pyrrhotite in carbonaceous chondrites; 1975; Article; Journal; Nature; Herndon, J. M.; Rowe, M. W.; Larson, E. E.; Watson, D. E. |
| URL (THUMBNAIL): | http://pubs.er.usgs.gov/thumbnails/outside_thumb.jpg |
| URL (DIGITAL OBJECT IDENTIFIER): | http://dx.doi.org/10.1038/253516a0 |
| Date Other: | Tue, 28 Sep 2010 23:09 -0500 |
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