中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300

文献类型:期刊论文

作者Hsu, Weibiao1; Zhang, Aicheng1; Bartoschweitz, Rainer2; Guan, Yunbin3; Ushikubo, Takayuki3; Kraehenbuehl, Urs4; Niedergesaess, Rainer5; Pepelnik, Rudolf5; Reus, Ulrich5; Kurtz, Thomas
刊名METEORITICS & PLANETARY SCIENCE
出版日期2008-08-01
卷号43期号:8页码:1363-1381
关键词ALEXANDRA RANGE 93069 HIGHLANDS SURFACE CRUST MOON EVOLUTION SAYH-AL-UHAYMIR-300 ANORTHOSITES PETROGENESIS DHOFAR-1180 PLAGIOCLASE
ISSN号1086-9379
英文摘要We report here the petrography. mineralogy. and geochemistry Of lunar meteorite Sayh al Uhaymir 300 (SaU 300). SaU 300 is dominated by it fine-grained crystalline matrix surrounding mineral fragments (plagioclase, pyroxene, olivine, and ilmenite) and lithic clasts (mainly feldspathic to noritic). Mare basalt and KREEPy rocks are absent. Glass melt veins and impact melts are present. indicating that the rock has been subjected to a second impact event. FeNi metal and troilite grains were observed in the matrix. Major element concentrations of SaU 300 (Al(2)O(3) 21.6 wt% and FeO S. 16 wt%) are very similar to those of two basalt-bearing feldspathic rei, regolith breccias: Calcalong Creek and Yamato (Y-) 983885. However. the rare earth element (REE) abundances and pattern of SaU 300 resemble the patterns of feldspathic highlands meteorites (e.g., Queen Alexandra Range (QUE) 93069 and Dar al Gani (DaG) 400), and the average lunar highlands crust. It has a relatively LREE-enriched (7 to 10 x CI) pattern with a positive Eu anomaly (similar to 11 x CI). Values of Fe/Mn ratios of olivine. pyroxene, and the bulk sample are essentially consistent With l lunar origin. SaU 300 also contains high siderophile abundances with a chondritic Ni/Ir ratio. SaU 300 has experienced moderate terrestrial weathering as its bulk Sr concentration is elevated compared to Other lunar meteorites, and Apollo and Luna samples. Mineral chemistry and trace clement abundances of SaU 300 fall within the ranges of lunar feldspathic meteorites and FAN rocks. SaU 300 is a feldspathic impact-melt breccia predominantly composed of feldspathic highlands rocks with a small amount of mafic component. With a bulk Mg# of 0.67, it is the most mafic of the Feldspathic meteorites and represents a lunar surface composition distinct from any other known lunar meteorites. Oil the basis of its low Th concentration (0.46 ppm) and its lack of KREEPy and mare basaltic components, the source region of SaU 300 could have been within a highland terrain, a great distance from the Imbrium impact basin, probably on the far side of the Moon.
WOS标题词Science & Technology ; Physical Sciences
学科主题Geochemistry & Geophysics
类目[WOS]Geochemistry & Geophysics
研究领域[WOS]Geochemistry & Geophysics
关键词[WOS]ALEXANDRA RANGE 93069 ; HIGHLANDS SURFACE ; CRUST ; MOON ; EVOLUTION ; SAYH-AL-UHAYMIR-300 ; ANORTHOSITES ; PETROGENESIS ; DHOFAR-1180 ; PLAGIOCLASE
收录类别SCI
语种英语
WOS记录号WOS:000261545400008
公开日期2011-12-30
源URL[http://159.226.72.40/handle/332002/1961]  
专题紫金山天文台_天体化学和行星科学实验室
作者单位1.Acad Sinica, Purple Mt Observ, Lab Astronchem & Plantery Sci, Lunar & Plantery Sci Ctr, Nanjing 210008, Peoples R China
2.Bartoschewitz Metorite Lab, D-38518 Gifhorn, Germany
3.Arizona State Univ, Dept Geol Sci, Tempe, AZ 85287 USA
4.Univ Bern, Abt Chem & Biochem, CH-3012 Bern, Switzerland
5.GKSS Forschungszent GmbH, Inst Kustenforsch, D-21502 Geesthacht, Germany
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GB/T 7714
Hsu, Weibiao,Zhang, Aicheng,Bartoschweitz, Rainer,et al. Petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300[J]. METEORITICS & PLANETARY SCIENCE,2008,43(8):1363-1381.
APA Hsu, Weibiao.,Zhang, Aicheng.,Bartoschweitz, Rainer.,Guan, Yunbin.,Ushikubo, Takayuki.,...&Kurtz, Paul.(2008).Petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300.METEORITICS & PLANETARY SCIENCE,43(8),1363-1381.
MLA Hsu, Weibiao,et al."Petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300".METEORITICS & PLANETARY SCIENCE 43.8(2008):1363-1381.

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来源:紫金山天文台

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