(1) セレスの明るい斑点の亜光化
A Nathues1, M Hoffmann1, M Schaefer1
1Max Planck Institute for Solar System Research, Goettingen, Germany.
Nature
|December 15, 2015
まとめ
輝く斑点と水氷の昇華がセレスで発見され,太陽系の"雪線"の向こうから物質が蓄積されたことを示唆しています. これは小惑星の地質学的な活動を示しています
科学分野:
- 惑星科学
- 天文地質学
- 太陽系探査
背景:
- 小惑星帯の最大の天体であるセレスは 異なる矮星です
- 木星と土星の氷の月とは違って セレスは潮力がなく 地質学的惰性を示唆しています
- 前回のセレスの水蒸気と結合した水の検出は,表面の氷の存在を暗示しました.
研究 の 目的:
- ローカル化された明るい領域の組成と活動を調査する
- 小惑星の地質学的な過程を理解するために
- セレスから集まった物質の起源を 特定するためです
主な方法:
- 衛星画像の分析
- 表面の組成のスペクトル検定
- 表面の特徴の昼間の変化の観測
主要な成果:
- セレスの明るい領域の発見,水素化マグネシウム硫酸と一致する.
- オカトールクレーターの明るい穴を特定し,おそらく水氷の昇華を示している.
- オクタークレーター内の昼間霧雲の観測,おそらく氷や塵の昇華から.
結論:
- セレスは地質学的な活動,特にオクタークレーターを示しています.
- 水の氷と特定の鉱物成分の存在は,太陽系の雪線を越えてセレスの物質を蓄積することを示唆しています.
- これらの発見は,小惑星帯に潮力が欠如している物体に対する地質学的惰性の仮定に異議を唱えます.
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