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Updated: Jul 28, 2026

Measuring Carbon-based Contaminant Mineralization Using Combined CO2 Flux and Radiocarbon Analyses
11:19

Measuring Carbon-based Contaminant Mineralization Using Combined CO2 Flux and Radiocarbon Analyses

Published on: October 21, 2016

火星の隕石 ALH84001 の炭酸塩の高温起源の可能性

R P Harvey1, H Y McSween

  • 1Department of Geological Sciences, Case Western Reserve University, Cleveland, Ohio 44106-7216, USA. rph@po.cwtu.edu

Nature
|July 4, 1996
PubMed
まとめ

火星隕石 アラン・ヒルズ 84001 カルボネートは,低温の水ではなく,衝突時の熱いCO2豊富な液体から形成された可能性が高い. このインパクトメタソマチズムは,それらの組成と鉱物区分を説明する.

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