van den Bergh S
Science. 1992 Oct 16;258(5081):421-4. doi: 10.1126/science.258.5081.421.
Modern distance determinations to galaxies were reviewed and placed on a uniform and self-consistent scale. Based on eight separate but not entirely independent techniques, the distance to the Virgo cluster was found to be 15.8 +/- 1.1 megaparsec. Twelve different determinations yield a Coma/Virgo distance ratio of 5.52 +/- 0.13 and hence a Coma distance of 87 +/- 6 megaparsec. With a cosmological redshift of 7210 kilometers per second, this gives a Hubble parameter H(0) (local) of 83 +/- 6 kilometers per second per megaparsec. From the velocity-distance relation of rich clusters of galaxies, the ratio of the value of H(0) (global) to the value of H(0) (local) was determined to be 0.92 +/- 0.08. In other words, the cluster data do not show a statistically significant difference between the local and global values of the Hubble parameter. If one nevertheless adopts this relation between H(0) (global) and H(0) (local), then the value of H(0) (global) is 76 +/- 9 kilometers per second per megaparsec. This observed value differs at the approximately 3sigma level (where sigma is the standard deviation of the distribution) from values in the range 36 less, similar H(0) less, similar50 kilometers per second per megaparsec, which are derived from stellar evolutionary theory in conjunction with standard cosmological models with a density parameter (Omega) that is equal to 1 and a cosmological constant (lambda) that is equal to 0.
对星系的现代距离测定进行了回顾,并将其置于一个统一且自洽的尺度上。基于八种不同但并非完全独立的技术,发现室女座星系团的距离为15.8±1.1百万秒差距。十二种不同的测定得出后发座/室女座星系团的距离比为5.52±0.13,因此后发座星系团的距离为87±6百万秒差距。宇宙学红移为每秒7210千米,由此得出哈勃参数H(0)(局部)为每秒每百万秒差距83±6千米。根据富星系团的速度 - 距离关系,确定H(0)(全局)与H(0)(局部)的值之比为0.92±0.08。换句话说,星系团数据并未显示出哈勃参数的局部值和全局值之间存在统计学上的显著差异。然而,如果采用H(0)(全局)与H(0)(局部)之间的这种关系,那么H(0)(全局)的值为每秒每百万秒差距76±9千米。这个观测值与从恒星演化理论结合密度参数(Ω)等于1且宇宙学常数(λ)等于0的标准宇宙学模型得出的每秒每百万秒差距36至50千米范围内的值在大约3σ水平(其中σ是分布的标准差)上存在差异。