彗星9P/テンペル1の親揮発物質:衝突前と衝突後
Michael J Mumma1, Michael A DiSanti, Karen Magee-Sauer
1Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. michael.j.mumma@nasa.gov
まとめ
テンプル11彗星
科学分野:
- 惑星科学は惑星科学である.
- 彗星科学 彗星科学
- アストロケミストリー アストロケミストリー
背景:
- 木星系彗星は,初期の太陽系についての洞察を与えてくれます.
- 彗星の揮発性組成は,起源と進化の経路を明らかにすることができます.
研究 の 目的:
- テンペル1彗星の親揮発性物質の豊富さを定量化するために.
- テンペル1の組成をオート雲彗星と比較するために.
- 彗星の氷の起源を調査する.
主な方法:
- 高分散赤外線スペクトロスコーピー (2.85.0マイクロメートル).
- 8つの親揮発性物質の定量化:H2O,C2H6,HCN,CO,CH3OH,H2CO,C2H2,CH4について
主要な成果:
- エタンの豊富さは,衝突後に大幅に増加した.
- メタノールとシアン化水素の濃度は,衝突後も変わらない.
- テンペル1のエジェクタはオート雲彗星と類似しているが,メタノールとアセチレンが少ない.
結論:
- テンペル1の揮発性氷とオート雲彗星は,元惑星円盤の共通の起源を共有している可能性が高い.
- インパクトイベントは,テンペル1の揮発性プロフィールを変化させた.
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