InSightの地震データから見た火星の上層マントルの構造
Amir Khan1,2, Savas Ceylan3, Martin van Driel3,4
1Institute of Geophysics, ETH Zürich, Zürich, Switzerland. akhan@ethz.ch.
まとめ
火星
科学分野:
- 地震学
- 惑星科学
- 地理学
背景:
- インサイトは火星の地震データを 2年間収集してきました
- 火星の内部構造と熱化学的状態を理解することは 惑星科学にとって極めて重要です
研究 の 目的:
- 火星の内部構造を 地震データを用いて 800キロメートルまで縮小します
- 火星の地殻の熱的石層と 熱の生成を調査する
主な方法:
- 8つの火星地震からの直接 (PとS) と表面反射 (PP,PPP,SS,SS) のボディウェーブ相の分析.
- 地震制約と地力学モデルを統合する.
主要な成果:
- 地球に比べて火星の熱層が 大きく厚くなることを示唆する 低速度地帯を特定した
- テレシーミック距離で S波の弱い影を観測した
- 火星地殻の熱生成元素の濃縮を予測した (13-20倍原始マントル).
結論:
- 火星の内部構造は 厚く冷たい石層で特徴付けられています
- 火星の地殻は 熱を生成する元素に 豊富に含まれていて 予想を上回っています
- この濃縮は,火星の表面熱流が 適度から高くなるのに寄与しています
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