セレスの水性変化したレゴリット内の広範囲の水氷:核スペクトロスコーピーの証拠
T H Prettyman1, N Yamashita2, M J Toplis3
1Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719-2395, USA. prettyman@psi.edu.
まとめ
矮惑星セレスの表面元素の組成は,過去の水質変化と氷岩の分断の可能性を示しています. 表面下では長期にわたる氷の存続を 示唆しています
科学分野:
- 惑星科学
- 天文地質学
- 天体化学
背景:
- 矮星セレスの表面の構成は 地質の歴史と揮発性物質に関する 重要な洞察を与えてくれます
- 規則石の組成を理解することは,水性変化と内部進化のプロセスを解読するのに不可欠です.
研究 の 目的:
- セレスの表面元素の組成 (水素,鉄,カリウム) を決定する.
- セレスのレゴリット氷の含有量と水性変化の歴史を制限する.
- 氷岩の分裂と内部進化を調査する
主な方法:
- NASAのドーンミッションの 核スペクトロスコピーのデータ分析
- セレスの表面における元素濃度の定量化.
主要な成果:
- 表面材料はセレスの内部で水分処理の証拠を示しています.
- 炭素を含有するセレスのレゴリズムは水素濃度が高いが,炭酸コンドライトと比較して鉄濃度が低い.
- 水素濃度が高い中高緯度地域では 地下水の氷が豊富にあることがわかります
結論:
- セレスの表面の組成は 氷岩の分断が わずかに起こったことを示しています
- 地表の氷は広範囲に存在し 何十億年もの間 存続しています
- この発見はセレスの氷の安定性の理論モデルを 裏付けている.
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