- 1610: Galileo
- 1676: Ole Rømer
- 1687: Isaac Newton
- 1781: William Herschel
- 1838: Friedrich Bessel
- 1861: William and Margaret Huggins
- 1912: Henrietta Leavitt
- 1917 Einstein
- 1920: Harlow Shapley
- 1929 Edwin Hubble
- 1948: Ralph Alpher
- 1949: Fred Hoyle
- 1963: Maarten Schmidt
- 1964: Arno Penzias and Robert Wilson
- 1978: Vera Rubin and Kent Ford
- 1989: Margaret Geller and John Huchra
- 1992: John Mather and George Smoot
- 1995: Robert Williams
- 1998: Saul Perlmutter and Brian Schmidt
- 2010: Wendy Freedman
Milky Way Galaxy
This diagram shows the major features of our Milky Way galaxy as viewed from the side. Viewed from above, the galactic disk is shaped like a pinwheel, with a central bulge. About 150 globular clusters are scattered in a sphere, forming a halo. Shapley assumed that the halo surrounded the center of the galaxy. By plotting distances to each cluster he was able to establish the center locate the Sun. The result was that the Sun and its family of planets, including Earth, are located in the disk about two thirds of the way from the galactic center.