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小惑星のペアの形成は,回転分裂による
P Pravec1, D Vokrouhlický, D Polishook
1Astronomical Institute AS CR, Fricova 1, CZ-25165 Ondrejov, Czech Republic. ppravec@asu.cas.cz
Nature
|August 27, 2010
まとめ
小惑星のペアは,親小惑星が急速に回転し,分裂する回転分裂によって形成されます. このプロセスは,観測された質量比とスピン周期を説明し,二重小惑星形成の新しいモデルをサポートします.
科学分野:
- * 惑星科学 (惑星科学)
- * 天文学 (アストロノミー)
- * 天体物理学
背景:
- *最近発見された小惑星のペアは,類似の太陽中心の軌道を共有しているが,重力的に結合していない.
- * 過去の軌道分析では,穏やかな分離が示されましたが,明確な形成メカニズムはありませんでした.
- * 回転分裂が仮説として提唱され,特定の質量比と回転周期が予測された.
研究 の 目的:
- * 小惑星のペアの形成メカニズムを調査する.
- * 小惑星のペアの性質を分析することによって,回転分裂仮説を検証する.
- * 核分裂の臨界質量比とスピン周期の関係を決定する.
主な方法:
- * 小惑星のペアのサンプルをフォトメトリックで観測した.
- * 小惑星ペアの回転周期と質量比を測定した.
- * データを分析して,主体回転周期と質量比を相関させた.
主要な成果:
- * 質量比が0.2を下回る小惑星の原発は,急激な回転を示し,重要な分裂速度に近づいています.
- * 質量比が0.2に近づくにつれ,プライマリーのスピン周期が長くなっていく.
- * 質量比が0.2を超える小惑星のペアは観測されなかった.
結論:
- *この発見は,小惑星のペアの主要な形成メカニズムとして,回転分裂を支持する.
- * 観測された質量比とスピン周期の関係は,分裂予測と一致しています.
- * 質量比が0.2以上のシステムには,破壊のための十分なエネルギーがなく,その欠如を説明します.
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