典型文献
Tungsten Isotopic Constraints on the Nature of Earth's Accreting Materials
文献摘要:
Tungsten isotope is a powerful tracer for the Earth's accreting materials because of the distinct W isotope compositions of the non-carbonaceous meteorites and carbonaceous meteorites.To better understand the evolution of the early Earth,here we calculated the expected μ183W of the bulk silicate Earth for different assumed compositions of the proto-Earth's mantle,the Moon-forming giant impactor,and the late veneer using a Monte Carlo approach.The result shows that the proto-Earth likely has a non-carbonaceous composition,while the carbonaceous chondrite-like materials were delivered to the Earth at the late stages of accretion.The predicted difference in μ183W values between the bulk silicate Earth and the non-carbonaceous meteorites of the scenarios assuming a pure carbonaceous composition for the giant impactor is slightly bigger than that of the scenarios assuming either a pure non-carbonaceous or a mixed carbonaceous-non-carbonaceous composition for the giant impactor(~5 ppm versus~2 ppm).The ancient mantle reservoir that partially lacks the late veneer with carbonaceous composition should have a negative μ183W value(from-3 to 0).Uncertainties introduced by the cosmogenic effects and mass-independent fractionation should be concerned during the high precision measurement ofμ183W for meteorites and ancient terrestrial samples in further work.
文献关键词:
中图分类号:
作者姓名:
MEI Qingfeng;YANG Jinhui
作者机构:
State Key Laboratory of Lithospheric Evolution,Institute of Geology and Geophysics,Chinese Academy of Sciences,Beijing 100029,China;College of Earth and Planetary Sciences,University of Chinese Academy of Sciences,Beijing 100049,China
文献出处:
引用格式:
[1]MEI Qingfeng;YANG Jinhui-.Tungsten Isotopic Constraints on the Nature of Earth's Accreting Materials)[J].地质学报(英文版),2022(04):1213-1220
A类:
Accreting,accreting,183W,veneer
B类:
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AB值:
0.469524
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