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Two-stage polybaric formation of the new enriched, pyroxene-oikocrystic, lherzolitic shergottite, NWA 7397

机译:新富集的辉石-高锰酸钙,锂沸石斜辉石的两阶段多气压形成,NWA 7397

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Northwest Africa (NWA) 7397 is a newly discovered, enriched, lherzolitic shergottite, the third described example of this group. This meteorite consists of two distinct textural lithologies (1) poikilitic—comprised of zoned pyroxene oikocrysts, with chadacrysts of chromite and olivine, and (2) nonpoikilitic—comprised of olivine, low-Ca and high-Ca pyroxene, maskelynite, and minor abundances of merrillite, spinel, ilmenite, and pyrrhotite. The constant Ti/Al ratios of pyroxene oikocrysts suggests initial crystallization of the poikilitic lithology at depth (equivalent to pressures of approximately 10 kbar), followed by crystallization of the nonpoikilitic lithology at shallower levels. Oxygen fugacity conditions become more oxidizing during crystallization ranging from fO_2 conditions of approximately QFM-2 to QFM-0.7. Magma calculated to be in equilibrium with the major rock-forming minerals is LREE-enriched relative to depleted or intermediate shergottites and has flat overall profiles. Therefore, we suggest that the parental magma for NWA 7397 had sampled an enriched, oxidized, Martian geochemical source, similar to that of other enriched basaltic and olivine-phyric shergottites. We present a polybaric formation model for the lherzolitic shergottite NWA 7397, to account for the petrologic constraints. Three successive stages in the development of NWA 7397 are discussed (1) formation of a REE-enriched parental magma from a distinct Martian mantle reservoir; (2) magma ponding and development of a staging chamber concomitant with initial crystallization of the poikilitic lithology; and (3) magma ascent to the near surface, with entrainment of cumulates from the staging chamber and subsequent crystallization of the nonpoikilitic lithology en route to the surface.
机译:西北非洲地区(NWA)7397是新发现的,富集的鳞片钙锌锰矿,这是该组的第三个例子。该陨石由两种截然不同的结构岩性组成:(1)坡辉石岩-由带状辉石的蛇纹石组成,具有铬铁矿和橄榄石的cha石,以及(2)非坡辉石岩-由橄榄石,低钙和高钙辉石,蒙脱石和少量的丰度组成蒙脱石,尖晶石,钛铁矿和黄铁矿。辉石o晶的Ti / Al比率恒定表明在深度(等效于约10 kbar的压力)下初始的微晶岩性结晶,然后在较浅的水平开始非微晶岩性结晶。氧逸度条件在结晶过程中变得更加氧化,范围从大约QFM-2到QFM-0.7的fO_2条件。计算得出与主要成岩矿物处于平衡状态的岩浆相对于贫化或中间的斜方锰矿富含LREE,并且具有平坦的总体轮廓。因此,我们建议NWA 7397的母岩浆采样了富集,氧化的火星地球化学源,与其他富集的玄武岩和橄榄石质斜方岩相似。我们提出了一种斜长石斜云母NWA 7397的多气压形成模型,以解决岩石学上的限制。讨论了NWA 7397发展的三个连续阶段:(1)从一个独特的火星地幔储层中形成富含REE的父母岩浆。 (2)岩浆沉积和阶跃室的发展,同时伴随着岩性岩性的初步结晶; (3)岩浆上升至近地表,从阶跃腔室夹带堆积物,随后非钾长石岩性结晶至地表。

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