Pyroxenes in Serra de Magé: cooling history in comparison with Moama and Moore County |
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| Authors: | George E Harlow CE Nehru Martin Prinz G Jeffrey Taylor Klaus Keil |
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| Institution: | 1. Department of Mineral Sciences, American Museum of Natural History, New York, NY 10024 U.S.A.;2. Department of Geology, Brooklyn College of the City University of New York, Brooklyn, NY 11210 U.S.A.;3. Department of Geology and Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131 U.S.A. |
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| Abstract: | Single-crystal X-ray, optical, and microprobe study of pyroxenes in the Serra de Magéfeldspar cumulate eucrite indicate complex exsolution features from a slow cooling history. Two pyroxenes now exist: “low” orthohypersthene ( P21ca) as host ( ～82 vol.%) and augite ( C2/c) in four distinct habits. This pyroxene pair yields an apparent “equilibration” temperature of ～900°. These relations are typical for orthopyroxene of both the Stillwater and Kintoki-San types, indicating an original pigeonite pyroxene with a bulk composition En51Fs39Wo10. Variations in augite-hypersthene textural relationships suggest variable initial compositions from about Wo8 to Wo11. The bulk composition is intermediate to those of initial pigeonites in Moama and Moore County but the augite-hypersthene tie line is longer suggesting a slower cooling history. Our examinations of all three meteorites show that Serra de Magéaugite lamellae are as thick or thicker than those in the other meteorites, contrary to the measurement of Miyamoto and Takeda. The compositional data, textural relations, and existence of P21ca hypersthene suggest at least a comparable if not slower cooling history for Serra de Magé. |
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