コンドルールとコンドライトの形成条件
C M O'D Alexander1, J N Grossman, D S Ebel
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA.
まとめ
チョンドル (chondrules) は,太陽系初期に発生した水滴で,密集した自己引力領域で形成された可能性が高い. これは,それらのナトリウム含有量を説明し,コンドルールの形成と小惑星の発達を結びつける.
科学分野:
- 惑星科学は惑星科学である.
- 宇宙化学 (コスモケミストリー)
- 初期の太陽系進化について
背景:
- コンドルル (chondrules) は,原始的な隕石 (コンドライト) に豊富に存在する,ミリメートルのサイズのシリケート球体である.
- その形成には,太陽系内部の初期のエネルギープロセスが関与しているが,その条件は不明である.
- コンドルル形成は,塵と惑星粒子を結びつける重要なプロセスです.
研究 の 目的:
- コンドルルの形成条件を調査する.
- コンドルルの化学的特性,特に揮発性元素の豊富さを説明する.
- コンドルル形成と惑星小惑星形成を結びつけるために.
主な方法:
- コンドルルにおけるナトリウム濃度の分析.
- コンドルル形成環境のモデリング.
- モデル予測とコンドルル化学組成の比較.
主要な成果:
- 揮発性元素のナトリウムは,コンドルールの形成の間に恒常的な豊富さを示しています.
- 恒常ナトリウムは形成領域に高固体密度を必要とするため,自己引力環境を示唆する.
- このモデルは,他のコンドルールの化学特性を説明します.
結論:
- コンドルル形成は,自己重力,密度の高い領域で発生した可能性が高い.
- チョンドル形成と小惑星形成は,相互に関連したプロセスである可能性が高い.
- コンドルル形成の理解は,太陽系増殖の初期段階の洞察を提供します.
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