在太阳系早期极端的氧同位素比率
Jérôme Aléon1, François Robert, Jean Duprat
1Centre de Recherches Pétrographiques et Géochimiques, 15 rue Notre Dame des Pauvres, BP20, 54501 Vandoeuvre-les-Nancy, France. aleon2@llnl.gov
Nature
|September 16, 2005
概括
新的石颗粒揭示了极端的氧同位素比率,表明太阳辐射,而不是多颗恒星,形成了太阳系早期的构建块.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 天体物理学 天体物理学
背景情况:
- 早期太阳系材料的同位素组成,如石,为其起源提供了洞察力.
- 行星物质中的氧同位素变异与具有不同核合成或化学历史的成分混合有关.
- 石颗粒的极端同位素变化通常归因于太阳前恒星源.
研究的目的:
- 为了研究新发现的石颗粒中发现的极端同位素组成的起源.
- 确定负责早期太阳系构建块的同位素构成的核合成过程.
主要方法:
- 在石有机物中发现的丰富的富含的颗粒中分析氧和同位素组成.
- 观察到的同位素比率与来自恒星核合成和太阳辐射模型的预测进行比较.
主要成果:
- 发现有史以来最极端的18O/16O和17O/16O比率的富含二氧化的颗粒 (约. 10^-1). 这样一来,我们就有了10^-1).
- 这些颗粒呈现出太阳同位素组成.
- 氧和同位素都指向一个单一的核合成或加工事件.
结论:
- 观察到的同位素组成与单一的异国情调进化恒星或年轻太阳的能量粒子对环太阳气体的辐射一致.
- 这项研究支持太阳辐射假设,因为它与预测的成分和捕获机制更好地一致.
- 这一发现挑战了对太阳系早期极端同位素变化的多重恒星贡献的传统观点.
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