Open main menu

Kent Ford (astronomer)

W. [William] Kent Ford, Jr. (born 1931) is an astronomer involved with the theory of dark matter. He worked with scientist Vera Rubin, who used his advanced spectrometer in her studies of space and matter. This spectrometer allowed the pair to drastically change the way dark matter was viewed, by analyzing the various spectrums of light galaxies give off in different parts of their spirals. He received the 1985 James Craig Watson Medal for his work on image enhancement and galactic dynamics.[1]

WorkEdit

Imaging Tube DevelopmentEdit

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.

Observational AstronomyEdit

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.

See alsoEdit

NotesEdit

  1. ^ Awards: James Craig Watson Medal, United States National Academy of Sciences
  2. ^ M. A. Tuve, W. K. Ford, Jr., J. S. Hall, and W. A. Baum, "Results of Preliminary Tests of Cascaded Image Converters," Publications of the Astronomical Society of the Pacific, Vol. 70, No. 417, 1958, p. 592.
  3. ^ W. K. Ford, Jr., "Electronic Image Intensification", Annual Review of Astronomy and Astrophysics, vol 6, 1, Sept. 1968. Retrieved 29 March 2019.
  4. ^ David DeVorkin and Shaun Hardy, Interview with W. Kent Ford, Jr., 25 October 2013, Niels Bohr Library & Archives, American Institute of Physics, College Park, MD. Retrieved 29 March 2019.
  5. ^ V. C. Rubin and W. K. Ford, Jr., "Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions", Astrophysical Journal, vol. 159, February 1970, p.379. Retrieved 29 March 2019.
  6. ^ V. C. Rubin, W. K. Ford, Jr., & N. Thonnard, "Rotational properties of 21 SC galaxies with a large range of luminosities and radii, from NGC 4605 /R = 4kpc/ to UGC 2885 /R = 122 kpc/", Astrophysical Journal, Part 1, vol. 238, June 1, 1980, p. 471-487. Retrieved 29 March 2019.

ReferencesEdit

External SitesEdit