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Updated: Jun 24, 2026

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
太陽系内部の初期の進化:隕石の視点
C M O'D Alexander1, A P Boss, R W Carlson
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, N.W., Washington, DC 20015, USA.
まとめ
太陽系 (太陽系) とは
科学分野:
- 惑星科学は惑星科学である.
- 天体物理学 天体物理学
- 宇宙化学 (コスモケミストリー)
背景:
- 太陽系形成理論 太陽系形成理論
- 初期の太陽系進化について
- 隕石の組成と起源について
研究 の 目的:
- 太陽系固体の起源を調査する.
- 隕石の形成機構を決定する.
- 初期の太陽系プロセスのタイムラインを再構築する.
主な方法:
- 隕石の組成の分析
- 太陽系物質の放射線年代測定法による年代測定
- 原惑星円盤の進化のモデリング
主要な成果:
- 隕石の短命な放射性核酸は,エネルギー粒子による放射線を示唆している.
- カルシウムとアルミニウムが豊富なインクルージョンとコンドルールは,小惑星帯で形成された可能性が高い.
- Tタウリ円盤で形成されたコンドリート隕石は,より高い温度に関する記憶を潜在的に保持しています.
結論:
- 地球の水は,水を持つ小惑星や木星近くの氷の惑星系から発生した可能性が高い.
- 地球上の惑星の形成は,太陽星雲の拡散後に起こった.
- 太陽系の進化には円盤形成,双極ジェット,そしてその後の微分化が含まれていた.
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