メルキュアの若い火山活動に関する証拠は,第3回メッセンジャー・フライバイからのものです
Louise M Prockter1, Carolyn M Ernst, Brett W Denevi
1Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. Louise.Prockter@jhuapl.edu
まとめ
MESSENGER宇宙船のデータは,水星の初期の広範な火山活動を明らかにしています. 証拠は,爆発的な噴出孔を含む火山活動が,太陽系の後の歴史に潜在的に,かなりの期間続いたことを示唆しています.
科学分野:
- 惑星科学は惑星科学である.
- 火山学 火山学とは
- インパクトクラテリング (インパクトクラテリング)
背景:
- MESSENGER宇宙船は,水星の地質学的進化に関する重要なデータを提供した.
- 以前の観測は,水星の初期の火山活動を示していた.
研究 の 目的:
- メッセンジャー号の飛行データを分析し,水星の火山活動を理解する.
- 水星の地質学的特徴の起源とタイミングを調査する. 水星.
主な方法:
- MESSENGER宇宙船のフライトバイからの高解像度の画像の分析.
- 滑らかな平原や衝突盆地を含む表面特性のスペクトル分析.
- 火山の地形と衝撃構造の地質学的解釈.
主要な成果:
- 水星に浸透した初期の火山活動が確認された.
- 若い290キロメートルのピークリング盆地が発見され,そのスペクトルは,火山起源の平らな平原と区別されています.
- 明るい堆積物を持つ爆発性火山噴出孔の大きな候補者の特定.
結論:
- 水銀の火山活動は広範囲に広がり,長期間にわたって発生しました.
- ピークリング盆地内の火山平原は,盆地形成後の噴出火山活動を示しています.
- この発見は,水星での火山活動が,太陽系の歴史の後半まで続いた可能性があることを示唆している.
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