The water content and parental magma of the second chassignite NWA 2737: Clues from trapped melt inclusions in olivine
文献类型：期刊论文
| 作者 | He, Qi1; Xiao, Long1; Hsu, Weibiao1,2; Balta, J. Brian3; McSween, Harry Y.3; Liu, Yang3 |
| 刊名 | METEORITICS & PLANETARY SCIENCE
 |
| 出版日期 | 2013-03-01 |
| 卷号 | 48期号:3页码:474-492 |
| ISSN号 | 1086-9379 |
| 通讯作者 | He, Q (reprint author), China Univ Geosci, Planetary Sci Inst, Wuhan 430074, Peoples R China. Email: qihe_cug@yahoo.com |
| 英文摘要 | NWA 2737, the second known chassignite, mainly consists of cumulate olivine crystals of homogeneous composition (Fo=78.7 +/- 0.9). These brown colored olivine grains exhibit two sets of perpendicular planar defects due to shock. Two forms of trapped liquids, interstitial melts and magmatic inclusions, have been examined. Mineral assemblages within the olivine-hosted magmatic inclusions include low-Ca pyroxene, augite, kaersutite, fluorapatite, biotite, chromite, sulfide, and feldspathic glass. The reconstructed parental magma composition (A#) of the NWA 2737 is basaltic and resembles both the experimentally constrained parental melt composition of chassiginites and the Gusev basalt Humphrey, albeit with lower Al contents. A# also broadly resembles the average of shergottite parent magmas or LAR 06319. However, we suggest that the mantle source for the chassignite parental magmas was distinct from that of the shergottite meteorites, particularly in CaO/Al2O3 ratio. In addition, based on the analysis of the volatile contents of kaersutite, we derived a water content of 0.480.67 wt% for the parental melt. Finally, our MELTS calculations suggest that moderate pressure (approximately 6.8kb) came closest to reproducing the crystallized melt-inclusion assemblages. |
| 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] | NAKHLA SNC METEORITE ; MARTIAN METEORITES ; SHERGOTTY METEORITE ; PHYRIC SHERGOTTITES ; MINERAL CHEMISTRY ; HYDROGEN ISOTOPES ; PHASE-EQUILIBRIA ; OXIDATION-STATE ; MARS ; PETROGENESIS |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000316963200011 |
| 公开日期 | 2014-01-08 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/9894]  |
| 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.China Univ Geosci, Planetary Sci Inst, Wuhan 430074, Peoples R China 2.Chinese Acad Sci, Purple Mt Observ, Lab Astrochem & Planetary Sci, Nanjing 210008, Peoples R China 3.Univ Tennessee, Planetary Geosci Inst, Dept Earth & Planetary Sci, Knoxville, TN 37996 USA |
| 推荐引用方式 GB/T 7714 | He, Qi,Xiao, Long,Hsu, Weibiao,et al. The water content and parental magma of the second chassignite NWA 2737: Clues from trapped melt inclusions in olivine[J]. METEORITICS & PLANETARY SCIENCE,2013,48(3):474-492. |
| APA | He, Qi,Xiao, Long,Hsu, Weibiao,Balta, J. Brian,McSween, Harry Y.,&Liu, Yang.(2013).The water content and parental magma of the second chassignite NWA 2737: Clues from trapped melt inclusions in olivine.METEORITICS & PLANETARY SCIENCE,48(3),474-492. |
| MLA | He, Qi,et al."The water content and parental magma of the second chassignite NWA 2737: Clues from trapped melt inclusions in olivine".METEORITICS & PLANETARY SCIENCE 48.3(2013):474-492. |
入库方式： OAI收割
来源：紫金山天文台
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