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1 Dominion Astrophysical Observatory, National Research Council of Canada, 5071 West Saanich Road, Victoria, British Columbia, V8X 4M6, Canada
Modern distance determinations to galaxies were reviewed andplaced on a uniform and self-consistent scale. Based on eightseparate but not entirely independent techniques, the distanceto the Virgo cluster was found to be 15.8 ± 1.1 megaparsec.Twelve different determinations yield a Coma/Virgo distanceratio of 5.52 ± 0.13 and hence a Coma distance of 87 ±6 megaparsec. With a cosmological redshift of 7210 kilometersper second, this gives a Hubble parameter H0 (local) of 83 ±6 kilometers per second per megaparsec. From the velocity-distancerelation of rich clusters of galaxies, the ratio of the valueof H0 (global) to the value of H0 (local) was determined tobe 0.92 ± 0.08. In other words, the cluster data do notshow a statistically significant difference between the localand global values of the Hubble parameter. If one neverthelessadopts this relation between H0 (global) and H0 (local), thenthe value of H0 (global) is 76 ± 9 kilometers per secondper megaparsec. This observed value differs at the 3 level (where is the standard deviation of the distribution) from valuesin the range 36 H050 kilometers per second per megaparsec,which are derived from stellar evolutionary theory in conjunctionwith standard cosmological models with a density parameter ()that is equal to 1 and a cosmological constant () that is equalto 0.