默奇森的希博尼特颗粒中的短寿命核化物:证据表明太阳系进化
K K Marhas1, J N Goswami, A M Davis
1Physical Research Laboratory, Ahmedabad 380009, India.
概括
短暂的-10 (10Be) 在默奇森石的希博尼特颗粒中被检测到,这表明它起源于太阳星云中的能量粒子辐射. 这一发现有助于区分恒星核合成对早期太阳系固体的贡献.
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:
- 石中的短寿命核酸提供了关于太阳系形成的见解.
- 希波尼特颗粒是研究早期太阳系条件的关键矿物阶段.
研究的目的:
- 调查早期太阳系固体中短寿命核的存在和起源.
- 使用石中的同位素异常来限制核合成过程.
主要方法:
- 来自默奇森石的希波尼特颗粒的分析.
- 测量同位素组成,特别关注-10 (10B) 过量,归因于-10 (10Be) 衰变.
- 与预期的-26 (26Al) 和-41 (41Ca) 的丰度进行比较.
主要成果:
- 在hibonite粒中检测到过多的10B,与10Be衰变一致.
- 在研究的谷物中没有发现26Al或41Ca衰变的证据.
- 观察到的10Be的丰度可以通过能量粒子辐射来解释.
结论:
- 能量粒子辐射是早期太阳星云中10Be的可信来源.
- 缺少26Al和41Ca衰变产物表明,这些核化物可能起源于恒星来源,而不是粒子辐射.
- 这项研究有助于区分早期太阳系元素的核合成起源.
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