A window into atmospheric escape on early Mars provided by argon isotopes in a Martian meteorite

被引:3
作者
Willett, Chelsea D. [1 ]
Cassata, William S. [1 ]
Marks, Naomi E. [1 ]
机构
[1] Nucl & Chem Sci Div, Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA
关键词
Mars; Argon; Martian meteorite; Mars atmospheric escape; Noble gas; MASS FRACTIONATION; NOBLE-GASES; DECAY CONSTANTS; EARLY EVOLUTION; COMPONENTS; ORIGIN; CONSTRAINTS; ALH84001; SOLAR; WATER;
D O I
10.1016/j.gca.2022.04.017
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Novel analytical approaches to determining the trapped Ar-38/Ar-36 ratio of gases contained within Martian meteorites are presented and applied to the Martian regolith breccia Northwest Africa (NWA) 7034 and paired stone NWA 11220. The resulting data indicate that extensive mass-dependent fractionation of atmospheric Ar may have occurred within 150 million years of planetary formation, ostensibly as a result of diffusion-limited hydrodynamic escape. The inferred fractional loss of Ar and lighter atmospheric constituents exceeds 50%. These data suggest that volatiles derived from planetary outgassing and/ or impactors may dominate the present abundance of atmospheric Ar. (C) 2022 Elsevier Ltd. All rights reserved.
引用
收藏
页码:119 / 134
页数:16
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