火星の海のタイミングは海岸線変形による
Robert I Citron1,2, Michael Manga1,2, Douglas J Hemingway1,2
1Department of Earth and Planetary Science, University of California, Berkeley, Berkeley, California, USA.
Nature
|March 21, 2018
まとめ
古代の火星の海は 沿岸線によって証明されています 新しい研究によると これらの海岸線は タルシスの火山期に形成され その後ではなく 地質学的不一致を解決し 初期の火星の水を支えた
科学分野:
- 惑星科学
- 地理学
- 天体生物学
背景:
- 証拠によると 古代の火星の海は 北の平原の海岸線が 重要な指標でした
- これらの海岸線は 均等な表面から逸脱し 海洋仮説に異議を唱えます
- タルシスの形成後の真の極流動に関する以前の説明は,タルシスの赤道起源と矛盾しています.
研究 の 目的:
- 古代の火星の海岸線が 均等な表面から 偏っていることを説明するために
- 火星の地質モデルと海岸線を 調和させるため
- 火星の海洋形成のタイミングを タルシスの火山活動と比較する
主な方法:
- タルシスの位置によって生じる地殻変形の地質モデル化.
- 岸辺の地形の変化の分析
- モデルの結果と観察データの比較
主要な成果:
- 岸辺の地形の変化は,タルシスの位置による変形によって説明される.
- 海岸線は タルシスの位置づけ前と後に形成された
- これは,非均等可能性の海岸線の地質学的不一致を解決します.
結論:
- 火星の大洋は 惑星の歴史の初期に 谷のネットワークの形成と一致しました
- 海洋の進化は,タルシスの火山の発生と衰退と密接に関連しています.
- これは火星の初期の地質学,水文学,気候に重大な影響を及ぼします.
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