コンドルルとカルシウム・アルミニウムに富んだインクルージョンの鉛同位体年齢
Yuri Amelin1, Alexander N Krot, Ian D Hutcheon
1Department of Earth Sciences, Royal Ontario Museum, Toronto, ON M5S 2C6, Canada. yamelin@NRCan.gc.ca
まとめ
隕石に含まれるカルシウムとアルミニウムが豊富なインクルージョン (CAI) とコンドルールの形成は,何百万年にもわたって起こりました. この研究は,これらの初期の太陽系イベントの正確な年齢制限を提供します.
科学分野:
- 宇宙化学 (コスモケミストリー)
- 惑星科学は惑星科学である.
- ジオクロノロジー (Geochronology) について
背景:
- カルシウムとアルミニウムが豊富なインクルージョン (CAI) とコンドルールは,隕石の原始的な成分です.
- それらの形成のタイムラインを理解することは,初期の太陽系プロセスを解明するために非常に重要です.
研究 の 目的:
- CVコンドライトにおけるCAIの形成と,CRコンドライトにおけるコンドルールの形成の間の年齢間隔を正確に決定する.
- 初期の太陽系におけるCAIおよびコンドルル形成イベントの期間を制限するために.
主な方法:
- Acfer 059隕石のコンドルールの鉛-鉛同位年代測定.
- エフレモフカ隕石のCAIの鉛同位体年代測定.
- 最初の26Al/27Al比率の分析.
主要な成果:
- リード・リード・イソクロン年齢は4564.7 ±0.6万年前です.
- CV CAIの鉛同位体の年齢は4567.2 ± 0.6 Maである.
- これは,CV CAIとCRコンドルル形成の間の2.5 ± 1.2百万年 (My) の間隔を示し,イベントは少なくとも1.3 My.続きます.
結論:
- CAIとコンドルル形成は,太陽系初期の重要な期間をカバーしました.
- 決定された時間間隔は,26Al-26Mgの体系化に基づいた時系列と一致しています.
- これは,太陽系物質の年代測定における26Al-26Mgイソトープ比の年代的重要性を裏付けるものである.
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