セレスの表面に現地のH2Oを検出
Jean-Philippe Combe1, Thomas B McCord2, Federico Tosi3
1Bear Fight Institute, 22 Fiddler's Road, P.O. Box 667, Winthrop, WA 98862, USA. jean-philippe_combe@bearfightinstitute.com.
まとめ
科学者は水 (H2O) を小惑星セレスで発見しました 特にオクソクレーターです この発見は,氷や鉱物水素から,最近の水活動や形成を示唆しています.
科学分野:
- 惑星科学
- 天体生物学
- 地質学
背景:
- 矮星セレスの表面は 水酸化物質が豊富です
- 以前の観測では水蒸気排出が示されましたが,直接の水 (H2O) の検出はありませんでした.
- 理論によると セレスの表面の下には 水の氷が豊富にあるというのです
研究 の 目的:
- 小惑星セレスの表面に水 (H2O) の直接的な証拠を特定する.
- オクソクレーター内の特定の領域の組成を調べる
主な方法:
- Dawn宇宙船の可視赤外線 (VIR) マッピングスペクトロメーターを利用した.
- オクソクレーターの 低照明で高反射の領域から 分析したスペクトルデータです
- 一ヶ月間観察を行った.
主要な成果:
- オクソのクレーターで 明確な水吸収の特徴を検出しました
- この特徴を5回観察した
- H2O氷やミネラル水素として特定された候補材料.
結論:
- この発見は,水 (H2O) の最近の露出または形成を示しています.
- 露出したH2Oの氷は,現在の温度のために長期間持続する可能性が低い.
- ミネラル水素は,液体または氷水との長期間の相互作用を示唆しています.
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