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American astronomer who discovered the galactic distance scale using RR Lyrae and
Cepheid variables in 1918. He looked at variables in globular
clusters, noticed that they were spherically arranged about a point 20 kiloparsecs away, which he
correctly identified as the center of the galaxy (although the true distance, corrected for interstellar
extinction, in 10 kpc). He extrapolated distances to the Large Magellanic Cloud by observing
RR Lyrae and Cepheid Variables. All were
assumed to lie at the same distance, and he obtained their distances using parallax measurements. He published a
catalog of bright galaxies in 1932 with Adelaide Ames, showing that nearby
galaxies are not uniformly distributed.
Additional biographies: Bruce Medalists, Bonn

de Vaucouleurs, G. and de Vaucouleurs, A.
Reference Catalog of Bright Galaxies, Being the Harvard Survey of Galaxies Brighter than the 13th Magnitude of H. Shapley and A. Ames, Revised, Corrected, and Enlarged with Notes, Bibliography, and Appendices.
Austin, TX: University of Texas Press, 1964.
Shapley, H. Flights from Chaos: A Survey of Material Systems from Atoms to Galaxies. New York: McGraw-Hill, 1923.
Shapley, H. (Ed.). Source Book in Astronomy 1900-1950. Cambridge, MA: Harvard University Press, 1960.
© 1996-2007 Eric W. Weisstein
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