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MINERALOGY AND PETROGENESIS OF LUNAR MAGNESIAN GRANULITIC METEORITE NORTHWEST AFRICA 5744

机译:西北非厄立特里亚颗粒状陨石的矿物学和成岩作用5744

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摘要

Lunar meteorite Northwest Africa (NWA) 5744 is a granulitic breccia with an anorthositic troctolite composition that may represent a distinct crustal lithology not previously described. This meteorite is the namesake and first-discovered stone of its pairing group. Bulk rock major element abundances show the greatest affinity to Mg-suite rocks, yet trace element abundances are more consistent with those of ferroan anorthosites. The relatively low abundances of incompatible trace elements (including K, P, Th, U, and rare earth elements) in NWA 5744 could indicate derivation from a highlands crustal lithology or mixture of lithologies that are distinct from the Procellarum KREEP terrane on the lunar nearside. Impact-related thermal and shock metamorphism of NWA 5744 was intense enough to recrystallize mafic minerals in the matrix, but not intense enough to chemically equilibrate the constituent minerals. Thus, we infer that NWA 5744 was likely metamorphosed near the lunar surface, either as a lithic component within an impact melt sheet or from impact-induced shock.
机译:西北非洲月球陨石(NWA)5744是粒状角砾岩,具有钙硅钙铝石斜长石,可能代表了先前未描述的独特地壳岩性。这种陨石是其配对组的同名和最早发现的石头。块状岩石的主要元素丰度与镁套房岩石具有最大的亲和力,但微量元素的丰度与铁锰钙铁矿的那些更为一致。 NWA 5744中相对不充分的微量元素(包括K,P,Th,U和稀土元素)的含量相对较低,这可能表明其来自高空地壳岩性或不同于月球附近Procellarum KREEP地层的岩性混合物。 NWA 5744的与冲击有关的热和冲击变质作用强度足以使基质中的黑镁质矿物再结晶,但强度却不足以化学平衡组成矿物。因此,我们推断NWA 5744可能在月球表面附近发生了变质,可能是撞击熔体板中的石块成分,也可能是撞击引起的冲击。

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