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Articles
The Hubble Constant
1 The author is a professor, a senior astronomer, and an associate director of the Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138
The Hubble constant is the constant of proportionality between recession velocity and distance in the expanding universe. It is a fundamental property of cosmology that sets both the scale and the expansion age of the universe. It is determined by measurement of galaxy The Hubble constant is the constant of proportionality between recession velocity and development of new techniques for the measurements of galaxy distances, both calibration uncertainties and debates over systematic errors remain. Current determinations still range over nearly a factor of 2; the higher values favored by most local measurements are not consistent with many theories of the origin of large-scale structure and stellar evolution.
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Science. ISSN 0036-8075 (print), 1095-9203 (online)