U.S. astronomer whose studies of the structure of the Galaxy placed the Sun near the central plane of the Galaxy some 30,000 light-years away from the centre.
In 1913 Shapley using results given by the U.S. astronomer Henry N. Russell in 1912 put into practice Russell´s methods for finding the dimensions of stars in a number of binary systems from measurements of their light variations when they eclipse one another.
These methods remained the standard procedure for more than 30 years.
Shapley also showed that Cepheid variables cannot be star pairs that eclipse each other.
He was the first to propose that they are pulsating stars.
Shapley joined the staff of the Mt. Wilson Observatory Pasadena California (now part of the Hale Observatories) in 1914.
Utilizing the 60-inch reflecting telescope at Mt. Wilson he made a study of the distribution of the globular clusters in the Galaxy. These clusters are immense, densely packed groups of stars some containing as many as 1,000,000 members.
He found that of the 100 clusters known at the time, one-third lay within the boundary of the constellation Sagittarius.
Utilizing the newly developed concept that variable stars (Cepheids and RR Lyrae stars) accurately reveal their distance by their period of variation and apparent brightness, he found that the clusters were distributed roughly in a sphere whose centre lay in Sagittarius.
Since the cluster assumed a spherical arrangement it was logical to conclude that they would form themselves about the centre of the Galaxy. From this conclusion and his other distance data Shapley deduced that the Sun lies at a distance of 50,000 light-years from the centre of the Galaxy.
His work which led to the first realistic estimate for the actual size of the Galaxy thus was a milestone in galactic astronomy.
In addition to his studies of the Galaxy he studied the neighbouring galaxies, especially the Magellanic Clouds, and found that galaxies tend to ccur in clusters which he called metagalaxies.
Shapley became professor of astronomy at Harvard University later of Harvard College Observatory (1921-52) and was made director emeritus and Paine Professor of Astronomy at Harvard in 1952.
His works include Star Clusters (1930), Flights from Chaos (1930), Galaxies (1943), The Inner Metagalaxy (1957) and Of Stars and Men...(1958).