相关实验视频
Updated: Jan 21, 2026

08:18
Three-Dimensional Reconstruction of Orbital Fractures
Published on: May 16, 2025
637
围绕银河系中心超大质量黑洞运行的恒星S0-2的相对红移
Tuan Do1, Aurelien Hees2,3, Andrea Ghez3
1Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA. tdo@astro.ucla.edu.
概括
天文学家通过观察银河系中心的恒星S0-2来测试爱因斯坦的相对论. 这颗恒星的红移证实了广义相对论的预测,
科学领域:
- 天体物理学
- 一般相对论
- 黑洞物理
背景情况:
- 一般相对论预测超大质量黑洞附近的恒星会出现相对红移.
- 银河系中心的恒星S0-2围绕着一个超大质量黑洞射手座A*运行.
研究的目的:
- 通过对S0-2恒星的观测来测试广义相对论的预测.
- 在接近超大质量黑洞的过程中测量S0-2的相对红移.
主要方法:
- 从1995年到2018年的S0-2的综合光谱和天文测量测量.
- 分析了S0-216年的轨道和接近黑洞的数据.
- 使用参数Y量化红移.
主要成果:
- 检测到了特殊相对论和重力红移的组合.
- 测量红移参数Y = 0.88 ± 0.17.
- 结果与广义相对论 (Υ = 1) 一致.
结论:
- 这些观测支持广义相对论对超大质量黑洞附近恒星轨道的预测.
- 一个牛顿模型 (Υ = 0) 被排除在5σ的统计意义之外.
- 这项研究为强大的引力场的相对论效应提供了有力的证据.
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