The Age and Size of the Universe
- 16 October 1992
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 258 (5081) , 421-424
- https://doi.org/10.1126/science.258.5081.421
Abstract
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 H0 (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 H0 (global) to the value of H0 (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 H0 (global) and H0 (local), then the value of H0 (global) is 76 ± 9 kilometers per second per megaparsec. This observed value differs at the ∼3σ level (where σ is the standard deviation of the distribution) from values in the range 36 ≲ H0 ≲50 kilometers per second per megaparsec, which are derived from stellar evolutionary theory in conjunction with standard cosmological models with a density parameter (Ω) that is equal to 1 and a cosmological constant (λ) that is equal to 0.Keywords
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This publication has 35 references indexed in Scilit:
- The large-scale velocity field beyond the local superclusterThe Astrophysical Journal, 1992
- The Hubble ConstantScience, 1992
- Systematic effects in lens inversions - Aleph(1) exact models for 0957 + 561The Astrophysical Journal, 1991
- The Global Hubble ConstantAustralian Journal of Physics, 1990
- Astronomical Imaging with Infrared Array DetectorsScience, 1988
- Multivariate analysis of elliptical galaxies in different environmentsThe Astrophysical Journal, 1986
- Hubble's constant and exploding carbon–oxygen white dwarf models for Type I supernovaeNature, 1985
- Can the Hubble constant be determined from H II region diametersThe Astrophysical Journal, 1980
- The determination of Q[SUB]0[/SUB] using X-ray and microwave observations of galaxy clustersThe Astrophysical Journal, 1978
- Direct observations of th large-scale distribution of galaxies.The Astrophysical Journal, 1976