相关实验视频
Updated: Jul 8, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
概括
天文学家使用多种方法确定了星系距离,产生了当地哈勃参数83 km/s/Mpc. 这个对宇宙学至关重要的值与全球测量结果一致,但与一些理论模型形成鲜明对比.
科学领域:
- 宇宙学和银河系外天文学.
- 确定宇宙距离的方法
- 测量哈勃参数的测量方法
背景情况:
- 准确的宇宙距离对于理解宇宙膨胀速度至关重要.
- 以前的距离测量显示出显著的分散,需要统一的尺度.
研究的目的:
- 为现代银河系距离测定建立一个统一和自相一致的尺度.
- 使用多种独立的技术来导出哈勃参数 (H(0) 的精确值.
主要方法:
- 审查和整合八种不同的距离测定技术.
- 计算到处女座和昏迷星系团的距离.
- 对丰富星系团的速度与距离关系的分析.
主要成果:
- 到处女座星团的距离被确定为15.8 ± 1.1 Mpc.
- 发现Coma星团距离为87 ± 6 Mpc.
- 计算出一个局部哈勃参数 (H(0) 局部值为83 ± 6公里/秒/Mpc,总值 (H(0) 全球值为76 ± 9公里/秒/Mpc.
结论:
- 这项研究为银河系外距离提供了一个强大的,统一的尺度.
- 哈勃导出的参数值在本地和全球测量之间是一致的.
- 结果与某些宇宙学模型预测的哈勃参数值存在统计学上显著的差异.
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