地化学:Pbイソトープが核形成の時期をどの程度把握できるのか?
1Department of Earth Sciences, Laurentian University, Sudbury, Ontario P31 6B5, Canada.
Nature
|November 3, 2006
まとめ
惑星核の形成は,おそらく3500万年以内に急速に発生し,長期にわたる2段階のプロセスを示唆するモデルに挑戦しました. 鉛イソトープデータの新しい分析は,初期の地球の増殖と微分を裏付けています.
科学分野:
- 地化学と惑星科学:惑星の核形成と増殖のタイミングとメカニズムを調査する.
背景:
- 地球の初期の歴史のモデルは,核形成の時間スケールを理解することに依存しています.
- 以前の研究では,ボルンガム (W) と鉛 (Pb) のクロノメーターに基づく2段階のコア形成が示唆されており,これは長期にわたるプロセスを暗示しています.
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