火星の核の地震検出
Simon C Stähler1, Amir Khan2,3, W Bruce Banerdt4
1Institute of Geophysics, ETH Zürich, Zürich, Switzerland. simon.staehler@erdw.ethz.ch.
まとめ
火星
科学分野:
- 惑星科学
- 地震学
- 地理学
背景:
- 惑星の内部構造は 地質学史の洞察を与えてくれます
- 火星の核を理解することは 進化にとって極めて重要です
研究 の 目的:
- 火星の液体金属核の 半径を決定する
- 火星の内部の組成と鉱物を推測する
主な方法:
- InSightデータを用いてコアマントルの境界からの地震波反射の分析.
- 地震と地質学的データの逆転
主要な成果:
- 火星の液体金属核の半径を 1830 ± 40 km に制限した.
- 核の平均密度は5.7〜6.3g/cm3で,軽い元素の含有量を示しています.
- 火星のマントルは地球の上層マントルに似ているが,ブリッジマニットが支配する下層マントルが欠けている.
結論:
- 火星は大きく 軽い元素に富んだ核を持っています
- 内部の構造は,地球と比較してマントルの組成の違いを示唆しています.
- 核影による地震データ制限は,将来の火星地震検出に影響を与える可能性があります.
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