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从衰变测量恒星年龄的测量
Nature
|February 24, 2001
概括
天文学家准确地确定了银河系的日期.
科学领域:
- 天文学和天体物理学
- 太空年代学是宇宙年代学.
- 恒星进化 恒星进化
背景情况:
- 最古老的恒星的年龄为宇宙提供了最小的年龄.
- 恒星的放射性约会使用放射性和稳定的同位素的丰富度比.
- 232Th是一种用于约会的长寿命放射性同位素,但238U提供了更高的精度.
研究的目的:
- 为了检测金属贫困恒星中单离子化 (238U) 的光谱线.
- 为了使用238U作为精确的宇宙年代计来测定银河系恒星的年龄.
- 为了建立一个更准确的宇宙年龄的下限.
主要方法:
- 对金属贫星CS31082-001.1.的光谱分析
- 在385.957nm的光谱线的检测.
- 观察和预测的同位素丰度比率的比较.
主要成果:
- 成功测量了385.957纳米单离子的光谱线.
- 在CS31082-001中确定了的丰富度为log ((U/H) = -13.7 +/- 0.14 +/- 0.12.
- 估计恒星的年龄为12.5 +/- 3 Gyr,为银河系提供了直接的年龄.
结论:
- 在CS31082-001中检测到238U线标志着恒星约会的重大进展.
- 这个宇宙计提供了迄今为止对银河系最直接的年龄确定.
- 理论和实验室数据的未来改进将提高宇宙年限的精度.
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