Constraints on Martian Chronology from Meteorites

被引：9

作者：

Vaci, Zoltan ^{[1
]}

Agee, Carl ^{[1
]}

机构：

[1] Univ New Mexico, Inst Meteorit, Albuquerque, NM 87131 USA

来源：

GEOSCIENCES | 2020年 / 10卷 / 11期

关键词：

Mars; geochemistry; radiogenic isotopes; geochronology; ND ISOTOPIC SYSTEMATICS; SM-ND; RB-SR; SNC METEORITES; DIFFERENTIATION HISTORY; PETROGENETIC MODEL; OXYGEN-ISOTOPE; CORE FORMATION; IGNEOUS ROCKS; MAGMA OCEAN;

D O I：

10.3390/geosciences10110455

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Martian meteorites provide the only direct constraints on the timing of Martian accretion, core formation, magmatic differentiation, and ongoing volcanism. While many radiogenic isotope chronometers have been applied to a wide variety of Martian samples, few, if any, techniques are immune to secondary effects from alteration and terrestrial weathering. This short review focuses on the most robust geochronometers that have been used to date Martian meteorites and geochemically model the differentiation of the planet, including Sm-147/Nd-143, Sm-146/Nd-142, Lu-176/Hf-176, Hf-182/W-182, and U-Th-Pb systematics.

引用

页码：1 / 15

页数：15

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