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Updated: Jun 23, 2026

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 15, 2013
火星の地殻の元素組成
Harry Y McSween1, G Jeffrey Taylor, Michael B Wyatt
1Planetary Geosciences Institute and Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996-1410, USA. mcsween@utk.edu
まとめ
火星 火星 火星 火星
科学分野:
- 惑星科学は惑星科学である.
- 地質化学 地質化学
- イグネウス Petrology (イグネウス・ペトロロジー) とは,イグネウス・ペトロロジー (イグネウス・ペトロロジー) とは
背景:
- 火星の地殻の構成は,その地質的進化と分化を理解するための鍵です.
- 宇宙船や隕石からの地球規模のデータは,岩殻の化学的性質の洞察力を提供します.
研究 の 目的:
- 火星の地質学的歴史を,火山状の地殻の組成を通して評価する.
- 惑星のマントルを理解するための火星隕石の代表性を評価する.
主な方法:
- グローバルな宇宙船データの分析.
- 火星の隕石組成の調査.
- 岩石化学の評価について.
主要な成果:
- 火星表面の岩は,主に,広範囲の部分的な融解から生じたトレイイート基岩で,気象の影響が最小限にある.
- 火星では,シリケ性,カルクアルカリ性,またはシリケが少ない岩石は稀です.
- 火星の隕石は,より古く,より豊富な地殻物質を正確に表現しないかもしれません.
結論:
- 地殻の組成は,限られた岩の種類とマントルの特定の融解過程を示している.
- 火星の隕石は,火星のマントルの構成や診断地化学を制限するのに理想的ではないかもしれません.
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