EH6 enstatite chondrites Northwest Africa 7976 and Northwest Africa 12945: Implications for EH chondrite metamorphism

被引:0
作者
Gray, Mabel L. [1 ,2 ]
Weisberg, Michael K. [1 ,2 ,3 ]
Jaret, Steven J. [1 ,2 ,3 ]
Ebel, Denton S. [1 ,2 ]
机构
[1] CUNY, Grad Ctr, Dept Earth & Environm Sci, New York, NY 10016 USA
[2] Amer Museum Nat Hist, Dept Earth & Planetary Sci, New York, NY 10024 USA
[3] CUNY, Kingsborough Coll, Dept Phys Sci, Brooklyn, NY USA
基金
美国国家航空航天局;
关键词
THERMAL HISTORY; SHOCK METAMORPHISM; IMPACT STRUCTURE; MELT ROCKS; CLASSIFICATION; METEORITES; PHASES; EL3;
D O I
10.1111/maps.14287
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The enstatite chondrite class is known to have complex thermal histories, often interpreted to include impact melting and shock metamorphism. Highly equilibrated (type 6) EH group enstatite chondrites are rare and thought to have formed through collisional heating. We studied two EH6 chondrites, NWA 7976 and NWA 12945, for their textural, chemical, and mineralogical characteristics. The samples we studied contain subhedral to anhedral grains of enstatite and plagioclase, suggesting solid-state recrystallization. They show low degrees of shock and no evidence of shock melting. Additionally, the ubiquitous occurrence of daubr & eacute;elite exsolution lamellae in troilite and the Ni content of schreibersite suggest slow cooling at greater burial depths in the parent body, rather than rapid cooling as a result of an impact event. Based on the characteristics and scarcity of type 6 EH chondrites, and the ubiquitous shock effects and melt rocks in the enstatite chondrite class, we conclude that the unshocked NWA 7976 and NWA 12945 were formed by heat derived from impact melt sheets, analogous to contact metamorphism.
引用
收藏
页码:51 / 63
页数:13
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