土星の奇妙な波紋状のCリング
M M Hedman1, J A Burns, M W Evans
1Department of Astronomy, Cornell University, Ithaca, NY 14853, USA. mmhedman@astro.cornell.edu
まとめ
土星 サターン
科学分野:
- 惑星科学は惑星科学である.
- 天文学 天文学
- リングダイナミクス リングダイナミクス
背景:
- 土星のC環は微妙な波紋を呈している.
- 同様の構造は以前,Dリングで観察されていた.
研究 の 目的:
- Cリング波紋の起源と特性を調査する.
- リングの傾きを引き起こしたイベントの性質を決定する.
主な方法:
- 2009年8月の土星のリングのエッジオン照明の分析.
- 波紋波長における放射的傾向の検討.
主要な成果:
- 2~20メートルの振幅と30~80キロメートルの波長を持つ波紋がCリング全体で検出されました.
- 構造の特徴は,傾いたリングの微分ノードル回帰からの形成を示唆しています.
結論:
- リングの傾きは,波紋化につながり,分散した惑星間破片による衝突の結果である可能性が高い.
- 瓦雲の質量は10^11から10^13キログラムと推定されている.
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