The Fountain Hills impact‐modified CB chondrite and thermal history of the CB asteroid |
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| Authors: | Michael K WEISBERG Denton S EBEL |
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| Institution: | 1. Department of Physical Sciences, Kingsborough College and Graduate School of the City University of New York, Brooklyn, New York 11235, USA;2. Department of Earth and Planetary Sciences, American Museum of Natural History, New York, New York 10024, USA |
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| Abstract: | Abstract— Fountain Hills is a metal‐rich chondrite with mineral and whole chondrite oxygen isotope compositions that suggest it is a CB chondrite. However, its petrologic characteristics suggest that it has been modified by shock and recrystallization to a greater degree than other CB chondrites. It differs texturally from the CB chondrites in that its metal is interstitial to the silicate and does not occur as discrete clasts as in the other CB chondrites. Portions of Fountain Hills appear to be recrystallized and it contains large (mm‐size) olivine rimmed by pyroxene. A characteristic of the CB chondrites is the presence of small sulfide blebs in large metal clasts and anomalously heavy (15N‐enriched) nitrogen often associated with metal surrounding the sulfide blebs, but Fountain Hills lacks sulfide and its nitrogen is relatively light. The differences between Fountain Hills and the other CB chondrites can be attributed to a secondary process, most likely impact‐melting and recrystallization, that overprinted its primary features and it is inferred that Fountain Hills is an impact‐modified CB chondrite. |
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