Detailed mineralogy and petrology of highly shocked poikilitic shergottite Northwest Africa 6342

被引:12
|
作者
Kizovski, Tanya V. [1 ,2 ]
Tait, Kimberly T. [1 ,2 ]
Di Cecco, Veronica E. [1 ]
White, Lee F. [1 ,2 ]
Moser, Desmond E. [3 ]
机构
[1] Royal Ontario Museum, Ctr Appl Planetary Mineral, Dept Nat Hist, 100 Queens Pk, Toronto, ON M5S 2C6, Canada
[2] Univ Toronto, Dept Earth Sci, 22 Russell St, Toronto, ON M5S 3B1, Canada
[3] Univ Western Ontario, Dept Earth Sci, 1151 Richmond St, London, ON N6A 5B7, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
LHERZOLITIC SHERGOTTITE; MULTICOMPONENT PYROXENES; MARTIAN METEORITE; OXYGEN FUGACITY; UPPER-MANTLE; THERMODYNAMICS; MARS; PETROGENESIS; METAMORPHISM; PETROGRAPHY;
D O I
10.1111/maps.13255
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
Northwest Africa (NWA) 6342 is an intermediate, poikilitic shergottite, found in Algeria in 2010. It is comprised of two distinct petrographic areas; poikilitic domains with rounded Mg-rich olivine chadacrysts enclosed by large low-Ca pyroxene oikocrysts, and a nonpoikilitic domain mainly comprised of subhedral olivine and vesicular recrystallized plagioclase. Oxygen fugacity conditions become more oxidizing during crystallization from the poikilitic to the nonpoikilitic domain (QFM-3.0 to QFM-2.2). As such, it is likely that NWA 6342 experienced a two-stage (polybaric) crystallization history similar to that of the enriched poikilitic shergottites. NWA 6342 also experienced relatively high levels of shock metamorphism in comparison to most other poikilitic shergottites as evidenced by the fine-grained recrystallization texture in olivine, as well as melting and subsequent crystallization of plagioclase. The recrystallization of plagioclase requires an extended period of postshock thermal metamorphism for NWA 6342 and similarly shocked intermediate poikilitic shergottites NWA 4797 and Grove Mountains 99027 most likely due to launch from Mars. The similarities in petrology, chemistry, and shock features between these three meteorites indicate that they have similar crystallization and shock histories; possibly originating from the same source area on Mars.
引用
收藏
页码:768 / 784
页数:17
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