原始的な太陽系物質と地球は,共通の初期 (142) Nd 量を持っています
1University of Western Ontario, Department of Earth Sciences, Centre for Planetary Science and Exploration, London, Ontario N6A 3K7, Canada.
Nature
|September 16, 2016
まとめ
初期の地球の組成は,カルシウムとアルミニウムが豊富な耐火性インクルージョン (CAI) と一致しており,コンドリティックなSm/Nd比を示唆しています. これは,隠された貯蔵庫を必要とせずにネオジミウム-142 (142Nd) のオフセットを解決します.
科学分野:
- 宇宙化学:サムリウム-ネオジミウム (Sm-Nd) 体系を用いて初期の太陽系の同位体進化を調査する.
- 惑星科学:イソトープ解析を通して惑星と惑星の初期の進化を制限する.
- 地化学:ネオジム-142 (142Nd) の変異を分析して惑星の形成と分化を理解する.
背景:
- ネオジム-142 (142Nd) 変異は初期惑星進化の洞察を提供しており,初期の円盤分布と短命のサマリウム-146 (146Sm) 崩壊から生じている.
- 以前の研究では,コンドリート隕石と地球の間の142Ndの豊富さのオフセットが認められ,核合成の変異や初期の地球の分化を含む解釈がなされた.
- カルシウムとアルミニウムに富んだ耐火性インクルージョン (CAI) とエンスタチトコンドライトは,初期の太陽系の同位体組成を再構築するための重要な材料です.
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