默奇森石中的贵重气体:可能是s过程核合成的遗迹
概括
原始石含有来自红巨星的前太阳尘埃粒,由独特的同位素图案证明. 这些发现表明,在太阳系形成之前,进化的恒星中发生了特定的核过程.
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:
- 像默奇森石一样的碳状石是太阳系原始材料.
- 石中离子同位素异常可以提供关于太阳前核合成的见解.
- 之前的研究已经确定了石中的各种前太阳成分.
研究的目的:
- 为了识别和描述Murchison石中的新同位素成分.
- 为了调查异常的贵重气体同位素丰富的起源.
- 为了将这些异常与特定的恒星核合成过程联系起来.
主要方法:
- 来自默奇森石的特定矿物质部分的贵重气体分析.
- 高温分级加热实验以释放被困的气体.
- 对,,和的同位素分析.
主要成果:
- 发现了一种新的用同位素128-132.2丰富的子成分.
- 识别了类似的,但较小的,缩在80和82的密同位素.
- 在同时释放的-22和-3中观察到异常丰富.
结论:
- 观察到的同位素模式强烈表明起源于恒星核合成,特别是红巨星中燃烧的s过程和/外.
- 这表明原始石中存在从红色巨星喷射出的前太阳尘埃粒.
- 这些发现有助于理解太阳前材料的多样性和太阳系早期的化学进化.
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