チャロンの表面組成:水氷の暫定的な識別
まとめ
1987年のハロン隠蔽の赤外線観測は,明確なスペクトルサインを明らかにしています. カロン・ハロンは,
科学分野:
- 惑星科学 惑星科学
- 天文学 天文学
- スペクトロスコーピーは,スペクトロスコーピーを用います.
背景:
- 冥王星とその衛星ハロンは,太陽系外部の重要な天体です.
- その表面の組成を理解することは,惑星形成モデルにとって極めて重要です.
研究 の 目的:
- 冥王星と相対的にハロンの表面の組成を決定する.
- チャロンに存在する特定の氷の存在を調査する.
主な方法:
- 1987年3月3日,ハロン・冥王星の隠蔽時の赤外線スペクトロスコーピー (1.5-2.35 μm) について.
- イベント前の/後のスペクトルフローを,イベント中のスペクトルフローから引く.
主要な成果:
- 冥王星とハロンの個別のスペクトルサインが得られた.
- チャロンの表面は,冥王星と比較してメタンの減少を示しています.
- シャロンは2.0μmでスペクトル的に黒く見え,水氷の強い吸収を示した.
結論:
- スペクトルデータは,チャロンの表面に水の氷が存在することを示唆しています.
- メタンの氷は,冥王星よりもハロンのほうが少ない.
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