How did Harlow Shapley use the period-luminosity relationship of RR Lyrae variable stars to determine the size of the Milky Way galaxy?
A) He found the distances to open clusters found throughout the disk of the galaxy.
B) He found the distances to individual variables free-floating in the halo of the galaxy.
C) He determined the proper motion of globular clusters in the outer disk of the galaxy.
D) He found the distances to globular clusters distributed about the centre of the galaxy.
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