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Updated: Apr 6, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
11.1K
コメタリー科学 CONSERTレーダーによって明らかになった67P/チュリュモフ・ゲラシメンコ内部の特性
Wlodek Kofman1, Alain Herique1, Yves Barbin2
1Université Grenoble Alpes, IPAG, F-38000 Grenoble, France (2) Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), F-38000 Grenoble, France.
まとめ
ラジオ波伝送による彗星核音響実験 (CONSERT) で,彗星67Pが発見された
科学分野:
- 惑星科学
- 彗星科学
- ラジオ科学
背景:
- 彗星は初期の太陽系の形成と進化の 洞察力を与えてくれます
- 彗星67P/チュリュモフ・ゲラシメンコへのフィラエ着陸器のミッションは,彗星の内部を研究するユニークな機会を提供しました.
研究 の 目的:
- 彗星67P/チュリュモフ・ゲラシメンコの内部構造を研究する.
- 彗星核の上の層の物理的性質を 決定するために
主な方法:
- ピラエの着陸機に搭載されたラジオ波伝送による彗星核音響実験 (CONSERT) を利用した.
- 彗星核を通る信号の伝播時間と形を分析した.
主要な成果:
- 上部
- 頭部
- 彗星67Pの領域は 10メートルスケールで均質です
- 約1. 27の平均許容性を決定しました.
- 粉と氷の比率は0.4~2.6で 毛細さは75%~85%と推定されています
結論:
- 彗星核の上の層は 顕著な同質性を表しています
- 粉塵の組成は炭酸性コンドライトと類似している.
- CONSERTのデータは,Philaeの着陸場所の不確実性を ~21×34メートルまで改善しました.
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