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Updated: Jul 25, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
相互作用するガス流と,彗星C/1996 B2 (Hyakutake) のコマに広がった揮発性源分布の証拠
W M Harris1, M R Combi, R K Honeycutt
1Space Astronomy Laboratory, University of Wisconsin, 1150 University Avenue, Madison, WI 53706, USA. wharris@sal.wisc.edu
まとめ
コメット・ハヤクタケ彗星
科学分野:
- 彗星科学は彗星科学である.
- 天文学 (astronomy) 天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは,天文学 (astronomy) とは
- 天体物理学 天体物理学
背景:
- 彗星C/1996 B2 (Hyakutake) の画像は,ガスと塵の明確な分布を示しています.
- 2つの弧状の分子共振放射の特徴は,内部の昏睡状態で観察されました.
研究 の 目的:
- ハヤクタケ彗星の内部昏睡の特徴の形態論を調査するために.
- 氷の粒が揮発性のある生産に与える貢献を理解するために.
主な方法:
- 彗星ヒヤクタケが地球に近付いたときの画像の分析.
- 観測データを解釈するためのモデルシミュレーション.
主要な成果:
- 内部コマで,ガスと塵の分離が観察されました.
- 核を囲む氷の粒の広大な領域の証拠.
- 氷を積んだ粒子の凝縮が,より明るい弧を説明し,揮発性産物の23%に貢献しています.
結論:
- 広大な氷の粒の領域は,彗星ヒヤクタケの揮発性生産に大きく貢献しています.
- モデルシミュレーションは,この氷の粒の領域の存在と活動を裏付けている.
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