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厚い雲の海王星のトロイの木馬とその色
Scott S Sheppard1, Chadwick A Trujillo
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road NW, Washington, DC 20015, USA. sheppard@dtm.ciw.edu
まとめ
天文学者は,高傾斜の海王星トロイの木馬,2005 TN53を発見し,厚い円盤群を明らかにしました. これは,海王星のトロイの木馬は"凍結"で捕獲され,in situで形成されていないことを示唆しています.
科学分野:
- 惑星科学は惑星科学である.
- 小惑星研究研究.
- 太陽系ダイナミクス 太陽系ダイナミクス
背景:
- 小惑星の性質は,巨大な惑星の形成と移住を制限する.
- トロイの木馬の小惑星は,惑星の半大軸の近くにラグランジアン点で軌道を回る.
- 海王星のトロイの木馬は,海王星の軌道を共有する小惑星の集団です.
研究 の 目的:
- 高傾斜の海王星トロイの木馬の発見を報告するために.
- ネプチューンのトロイの木馬の集団の分布と起源を特徴づけるために.
- ネプチューンのトロイの木馬と木星のトロイの木馬,カイパーベルトのオブジェクトを比較するために.
主な方法:
- 観測天文学を用いた小惑星2005 TN53の発見.
- 人口分布を決定するために軌道傾斜の分析.
- 表面の組成と進化の歴史を推測するための色彩測定.
主要な成果:
- 高傾斜の海王星のトロイの木馬2005 TN53.3の発見
- ネプチューン・トロイの木馬の厚いディスク分布の証拠.
- ネプチューンのトロイの木馬は,木星のトロイの木馬よりも潜在的に多い.
- ネプテュンのトロイの木馬は,わずかに赤い色を呈し,互いに似ていますが,カイパーベルトオブジェクトとは異なります.
結論:
- ネプチューン・トロイの木馬の厚い円盤は,海王星の惑星を支えている.
- フリーズイン (freeze-in) とは
- 捕まえるメカニズム.
- ネプテュンのトロイの木馬は,おそらく共通の形成と進化の歴史を共有しています.
- ネプチューンのトロイの木馬は,古典的なカイパーベルトオブジェクトとは,ダイナミックで構成的に異なる.
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