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DOI | 10.1038/s41561-019-0433-4 |
Tin isotopes indicative of liquid-vapour equilibration and separation in the Moon-forming disk | |
Wang, Xueying1; Fitoussi, Caroline1; Bourdon, Bernard1; Fegley, Bruce, Jr.2,3; Charnoz, Sebastien4 | |
2019-09-01 | |
发表期刊 | NATURE GEOSCIENCE
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ISSN | 1752-0894 |
EISSN | 1752-0908 |
出版年 | 2019 |
卷号 | 12期号:9页码:707-+ |
文章类型 | Article |
语种 | 英语 |
国家 | France; USA |
英文摘要 | The depletion in moderately volatile elements in the Moon relative to Earth and comparison of the isotope compositions of the Moon and Earth have placed important constraints on models of lunar formation. A liquid-vapour protolunar disk from a high-energy giant impact has been proposed to explain some of these constraints. Here we present high-precision tin isotope data for lunar rocks, measured by double-spike MC-ICP-MS (multicollector inductively coupled plasma mass spectrometry). The lunar rocks are enriched in light tin isotopes compared to the Earth (Delta Sn-127(/116)Moon-Earth = -0.48 +/- 0.15 parts per thousand). On the basis of our data and constraints on tin speciation, we show that this tin isotope fractionation is inconsistent with volatile loss from a lunar magma ocean. Instead, we propose a scenario with vigorous mixing between the protolunar disk and the Earth in high-energy conditions during the impact, followed by liquid-vapour equilibration and phase separation at around 2,500 K while the disk was cooling. This scenario is consistent with the depletion in moderately volatile elements and isotope composition of the Moon. |
领域 | 地球科学 ; 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000484058100009 |
WOS关键词 | TEMPERATURE VAPORIZATION BEHAVIOR ; BUILDING-BLOCKS ; CROSS-SECTIONS ; ORIGIN ; EARTH ; FRACTIONATION ; OXIDES ; CORE ; MARS ; ZN |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/186879 |
专题 | 地球科学 气候变化 |
作者单位 | 1.Univ Lyon, UCBL, CNRS, Lab Geol Lyon,ENS Lyon,UMR 5276, Lyon, France; 2.Washington Univ, Planetary Chem Lab, McDonnell Ctr Space Sci, St Louis, MO 63110 USA; 3.Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA; 4.Univ Paris Diderot, CNRS, UMR 7154, Inst Phys Globe Paris,Sorbonne Paris Cite, Paris, France |
推荐引用方式 GB/T 7714 | Wang, Xueying,Fitoussi, Caroline,Bourdon, Bernard,et al. Tin isotopes indicative of liquid-vapour equilibration and separation in the Moon-forming disk[J]. NATURE GEOSCIENCE,2019,12(9):707-+. |
APA | Wang, Xueying,Fitoussi, Caroline,Bourdon, Bernard,Fegley, Bruce, Jr.,&Charnoz, Sebastien.(2019).Tin isotopes indicative of liquid-vapour equilibration and separation in the Moon-forming disk.NATURE GEOSCIENCE,12(9),707-+. |
MLA | Wang, Xueying,et al."Tin isotopes indicative of liquid-vapour equilibration and separation in the Moon-forming disk".NATURE GEOSCIENCE 12.9(2019):707-+. |
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