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太阳前物质的各种超新星来源推断来自石中的同位素
Qingzhu Yin1, Stein B Jacobsen, Katsuyuki Yamashita
1Department of Earth and Planetary Sciences, Harvard University, Cambridge, Massachusetts 01238, USA.
Nature
|February 23, 2002
概括
原始石揭示了不同的恒星起源,因为它们的同位素成分与太阳平均值不同. 这表明来自多个超新星爆炸的物质有助于早期太阳系.
科学领域:
- 太空化学 太空化学
- 核天体物理学 核天体物理学
- 行星科学 行星科学
背景情况:
- 石中的太阳前物质显示不完整的均质化和低温处理,表明不同的恒星来源.
- 碳状地石代表了太阳系的平均组成,罕见的太阳前粒提供了起源的线索.
研究的目的:
- 为了研究散装碳状地铁的同位素组成.
- 为了确定这种组成是否与公认的平均太阳能值保持一致.
- 为了确定核合成过程和恒星来源,为早期太阳系材料做出贡献.
主要方法:
- 在散装碳状地铁体中分析 (Mo) 同位素组成.
- 流星数据与公认的平均太阳值进行比较.
- 核合成过程 (r过程和p过程) 的建模,以解释观察到的同位素变化.
主要成果:
- 大量的碳状地铁体呈现出不同于平均太阳值的同位素组成.
- 观察到的Mo同位素数据需要至少两个不同的r过程事件的贡献.
- 发现p-工艺材料的贡献与r-工艺贡献脱.
结论:
- 早期的太阳系包含来自不同恒星来源的物质,包括多个r过程事件和超新星的分离p过程物质.
- 这些发现与短寿命同位素的证据和金属贫乏恒星的元素分析一致,支持太阳系组件的复杂起源.
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