Kent Ford (astronomer)

Starting in 1955, when he was hired at the Carnegie Institute's Department of Terrestrial Magnetism, Ford worked on improving the electrostatic photomultiplier tube and developing it as an instrument for scientific work, and went on to pioneer the application of photomultiplier tubes as a sensitive focal-plane detector for astronomical applications,[2] resulting in the "Carnegie Image Tube".[3] The first tests of the astronomical applications of his barrier film tubes were done on the 26-inch refractor at the Naval Observatory in Washington, and later at the 40-inch telescope at the Naval Observatory in Flagstaff.[4] By making it possible for astronomical observations to be captured in electronic form, and thus easily transferred to digital form for analysis by computer, the technology revolutionized the data collection method of observational astronomy, and the technology continued to be widely used for astronomical observations until the development of CCD imagers in the 1980s.

In an important paper co-authored with astronomer Vera Rubin in 1970,[5] and a follow-up paper in 1980,[6] Rubin and Ford established that the orbits of stars around the center of galaxies (the "galaxy rotation curve") does not decrease with distance from the galactic center, as expected from Kepler's rotation law, but remains constant (or "flat") with distance. They deduced from this that galaxies contain a large fraction of their mass in the form of some non-luminous component, and calculated that most galaxies must contain about six times as much dark as visible mass. The name now given to this discovery is dark matter.