地球の異常 (142) Nd組成の核合成起源
C Burkhardt1,2, L E Borg3, G A Brennecka2,3
1Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago, Illinois 60637, USA.
Nature
|September 16, 2016
まとめ
地球のアクセシブルシリケートには,コンドライトよりもネオジミウム-142とネオジミウム-144の比率が高い. この違いは,初期の地球分化ではなく,ゆっくりとした中性子捕獲プロセスであるネオジミウムが過剰に存在しているため,大質量地球におけるコンドリティックなSm/Nd比を示唆している.
科学分野:
- 地化学
- 宇宙化学
- 惑星科学
背景:
- 大量シリケート地球の化学および同位体組成は,しばしばコンドライトを反映すると考えられています.
- しかし,アクセシブルな地球は,コンドライトと比較して (142) Nd / (144) Nd の比率が高くなります.
- この同位体オフセットは初期の地球分化に起因し,隠れたまたは失われた補完貯蔵庫を暗示しています.
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