Climate Change Data Portal
DOI | 10.1038/s41561-019-0433-4 |
Tin isotopes indicative of liquid–vapour equilibration and separation in the Moon-forming disk | |
Wang X.; Fitoussi C.; Bourdon B.; Fegley B.; Jr.; Charnoz S. | |
发表日期 | 2019 |
ISSN | 17520894 |
卷号 | 12期号:9 |
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 (Δ124/116SnMoon–Earth = −0.48 ± 0.15‰). 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. © 2019, The Author(s), under exclusive licence to Springer Nature Limited. |
语种 | 英语 |
scopus关键词 | cooling; isotopic composition; isotopic fractionation; lunar crust; Moon; separation; speciation (chemistry); tin |
来源期刊 | Nature Geoscience |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/124609 |
作者单位 | Laboratoire de Géologie de Lyon, ENS Lyon, CNRS UMR 5276, Université de Lyon, UCBL, Lyon, France; Planetary Chemistry Laboratory, McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University, Saint Louis, MO, United States; Institut de Physique du Globe de Paris, Sorbonne Paris Cité, CNRS UMR 7154, Université Paris Diderot, Paris, France |
推荐引用方式 GB/T 7714 | Wang X.,Fitoussi C.,Bourdon B.,等. Tin isotopes indicative of liquid–vapour equilibration and separation in the Moon-forming disk[J],2019,12(9). |
APA | Wang X.,Fitoussi C.,Bourdon B.,Fegley B.,Jr.,&Charnoz S..(2019).Tin isotopes indicative of liquid–vapour equilibration and separation in the Moon-forming disk.Nature Geoscience,12(9). |
MLA | Wang X.,et al."Tin isotopes indicative of liquid–vapour equilibration and separation in the Moon-forming disk".Nature Geoscience 12.9(2019). |
条目包含的文件 | 条目无相关文件。 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。