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分断された彗星73P/シュワスマン=ワッハマン3の構成が均一である
N Dello Russo1, R J Vervack, H A Weaver
1Space Department, The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, Maryland 20723-6099, USA. neil.dello.russo@jhuapl.edu
Nature
|July 13, 2007
まとめ
73P/Schwassmann-Wachmann 3の断片で研究された彗星の氷の組成は,驚くべき均一性を示しています. これは,彗星における観測された炭素鎖化学は,太陽の進化の結果ではなく,原始的なものであることを示唆している.
科学分野:
- 彗星科学は彗星科学である.
- アストロケミストリー アストロケミストリー
- 太陽系形成 太陽系形成について
背景:
- 彗星の揮発性氷の組成は,形成環境,貯蔵,太陽光処理によって大きく変化します.
- この多様性を理解するには,彗星核の化学を深く分析する必要があります.
- 以前の観察は,形成条件と進化的影響を評価する点で限られていた.
研究 の 目的:
- 彗星73P/シュワスマン=ワッハマン3の異なる断片の化学組成を調査する.
- 彗星の氷の組成における形成条件と進化過程の役割を評価する.
- 短周期彗星における深さによる組成の変動があるかどうかを判断する.
主な方法:
- 彗星73P/シュワスマン=ワッハマン3の2つの別々の断片の化学組成の分析
- 断片の組成を互いに比較し,より広い彗星集団と比較する.
- 彗星の既知の貯水池と関連して,揮発性氷の減少の評価.
主要な成果:
- 73P/Schwassmann-Wachmann 3の2つの断片は,非常に類似した化学組成を示した.
- この均一性は,短期彗星の予想される組成の多様性とは大きく対照的です.
- 彗星73P/シュワスマン=ワッハマン3は,他の彗星と比較して,高度に揮発性のある氷で枯渇しています.
結論:
- 73P/シュワスマン=ワッハマン3の断片の均一な組成は,短周期彗星における進化的処理の期待に挑戦している.
- 揮発性氷と炭素鎖化学の観測された枯渇は,進化的ではなく,原始的な起源を示唆しています.
- 彗星の氷の組成は,これまで考えられていたよりも初期の形成条件を反映しているかもしれません.
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