The Bovedy meteorite; mineral chemistry and origin of its Ca-rich glass inclusions
The Bovedy meteorite; mineral chemistry and origin of its Ca-rich glass inclusions
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博维迪陨石;
DOI:
10.1016/0016-7037(76)90220-9
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发表时间:
1976
影响因子:
5
通讯作者:
D. Jérôme
中科院分区:
文献类型:
--
作者:
A. Graham;A. J. Easton;R. Hutchison;D. Jérôme
The Bovedy meteorite fell on 25 April 1969 in Northern Ireland; the main mass of 4·94 kg was found at Bovedy (54°57′N, 06°37′W). It is an L3 chondrite with abundant chondrules clearly visible in hand specimen. Bulk chemical analyses are presented, the total Fe content being 22·5%. The olivines are homogeneous (Fa24) but the pyroxenes are not equilibrated (Fs8–28). Brown glass is common within chondrules but a clear glass of composition An85is present interstitially in a few orthopyroxene-rich (Fs17–28) chondrules. A bleb, 2 mm across, of clear glass, again of composition An85was found in one stone of the meteorite and in the glass five REE (rare earth elements), (La, Sm, Eu, Yb, Lu) were determined. The low REE abundances coupled with a large positive Eu anomaly are characteristic of plagioclase, but the finer details of the pattern suggest that this glass has a closer affinity to the lunar anorthosites than to plagioclases from lunar mare basalts or eucritic meteorites. There is also evidence that the magnitude of the Eu anomaly for plagioclases and anorthosites from extra-terrestrial sources is inversely related to trivalent REE content. The existence of anorthositic material and, as a consequence, a differentiated planetary body prior to the formation of the Bovedy meteorite is suggested.