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Updated: Dec 29, 2025

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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彗星67Pの軌道上の水氷サイクル
Gianrico Filacchione1, Fabrizio Capaccioni2, Mauro Ciarniello2
1INAF-IAPS, Institute for Space Astrophysics and Planetology, Rome, Italy. gianrico.filacchione@inaf.it.
Nature
|February 7, 2020
まとめ
彗星67P/チュリュモフ・ゲラシメンコは,その表面とコマで逆の季節的な色変化を示しています. 有機物質に富んだ塵はコマを赤くし 露出した氷は近日期の核表面を青くする
科学分野:
- 惑星科学
- 彗星科学
- 天体化学
背景:
- 彗星の活動は太陽の熱によって引き起こされ ガスと塵が放出されます
- 彗星のコマと核の性質は軌道全体で動的に進化する.
- 粉塵の粒子の色は成分 (有機,シリケート,水氷) と粒子の大きさによって異なります.
研究 の 目的:
- 彗星67P/チュリュモフ・ゲラシメンコの表面とコマの季節的な色サイクルを観察し分析する.
- 太陽熱,塵の組成,そして観測された色の変化との関係を調査する.
主な方法:
- 彗星67P/チュリュモフ・ゲラシメンコの観測のスペクトル解析
- コマと核の表面の色差を監視する.
主要な成果:
- コマと核の2つの異なる季節の色サイクルを観測した.
- 微細な有機物質と無形な炭素粒子の濃縮に起因する.
- 核の表面は 粉末が除去されるにつれて 純粋な氷の層の露出により 青い色が示されました
結論:
- 彗星の塵の組成と粒子の大きさはコマの色に大きな影響を与える.
- 季節の変化は,塵の除去,氷の昇華,そして表面の進化の間のダイナミックな相互作用を明らかにします.
- 太陽から遠く離れたところでは 表面の脱水と塵の再配置により 水の氷の量とコマの赤みが減少します
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