惑星系間の極端な衝突が,太陽のような恒星の周りの熱い塵の起源である
Inseok Song1, B Zuckerman, Alycia J Weinberger
1Gemini Observatory, 670 North A'ohoku Place, Hilo, Hawaii 96720, USA. song@gemini.edu
Nature
|July 22, 2005
まとめ
科学者たちは,若い恒星BD+20,307の周りに豊富な温かい塵を発見し,最近の小惑星衝突を示唆しました. この発見は,初期の惑星形成と小惑星帯の進化に関する手がかりを提供します.
科学分野:
- エクソプラネット科学 エクソプラネット科学
- 恒星系の進化 恒星系の進化
- 塵のダイナミクス
背景:
- 星座の光は,太陽系の小惑星の衝突から発生します.
- 星座塵に類似する温かい塵は,若い恒星の周りに稀である.
- 陸上の惑星の形成の証拠は,若い恒星系では捉え難いものでした.
研究 の 目的:
- 若い太陽型星の内部の熱い塵の存在を調査する.
- 初期の恒星系における塵の生成と小惑星衝突のプロセスを理解する.
主な方法:
- 太陽型星BD+20,307.7の観測について
- 星の周辺の塵の構成と量の分析.
主要な成果:
- BD+20,307.7周辺には,非常に多くの温かい小さなシリケート塵の粒子が検出されました.
- 塵の特徴は,近年,頻繁に,または惑星間衝突が起きたことを示唆しています.
結論:
- この発見は,BD+20,307.7.の地上の惑星形成地帯における惑星小惑星の衝突が活発であることを示している.
- 近くの惑星がこれらの惑星系の軌道を乱す可能性があり,観測された塵につながります.
- この発見は,惑星形成の初期段階についての珍しい洞察を与えてくれます.
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