Beginning with the Andromeda galaxy in the late 1960s, the astronomer Vera Rubin and her colleague Kent Ford measured how fast stars and gas clouds orbit at different distances from a galaxy’s centre. They expected the outer material to move slowly. It did not. In Andromeda, and then in galaxy after galaxy, the orbital speed stayed high all the way to the edge of what they could measure. The visible stars, gas and dust could not supply enough gravity to hold matter moving that fast in place.
Rubin and Ford published their Andromeda result in 1970, in a paper in the Astrophysical Journal. Over the following decade they extended the work, and by 1980 had measured the same pattern across twenty-one spiral galaxies. The consistency was the point. One odd galaxy could be explained away. Twenty-one could not.









