隕石の含有物中のモリブデンイソトープから太陽系の形成の天文学的背景
Gregory A Brennecka1,2, Christoph Burkhardt2, Gerrit Budde2,3
1Lawrence Livermore National Laboratory, Livermore, CA, USA. brennecka2@llnl.gov.
まとめ
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) は,太陽系の最初の固体であり,その誕生のタイムラインを提供します. 独特のモリブデンイソトープは 太陽の初期のTタウリ期で20万年以内に CAIが形成されたことを示唆しています
科学分野:
- 宇宙化学
- 天文学
- 惑星科学
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) は,太陽系で最も古い固体です.
- CAIは,太陽系形成の絶対時間スケールを設定します.
- 彼らの研究は天文学的な星形成の観測と 宇宙化学の分析を結びつけています
研究 の 目的:
- CAIの形成時代を調査する.
- 太陽系が形成された時のスケールを 調べるためだ
- 恒星の進化の中で太陽系の形成を文脈化するために.
主な方法:
- CAIにおけるモリブデン (Mo) の同位体組成の分析
- CAIの同位体データを原惑星円盤物質のモデルと比較.
- CAI形成のタイミングと恒星進化の相関
主要な成果:
- CAIは,原惑星円盤の材料の全範囲をカバーする幅広いモリブデン同位体組成を示しています.
- CAIの形成は20万年未満の短い期間に起こった.
- CAIの形成は,太陽が原星からTタウリ段階への移行と一致した.
結論:
- 太陽系の形成と蓄積は,CAI形成の時代に発生し,急速であった.
- CAIの形成は 恒星系と惑星系の進化の間の 重要なつながりです
- 太陽とその惑星の物質は,この短命な初期段階において,大部分が蓄積された.
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