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Encyclopedia Britannica



PICKERING, EDWARD CHARLES (1846- )

This article appears in Volume V21, Page 583 of the Encyclopedia Britannica.

Encyclopedia Britannica - Main :: PER-PIG
PICKERING, EDWARD CHARLES (1846- ) , American physicist and astronomer, was born in Boston on the 19th of July 1846. He graduated in 1865 at the Lawrence Scientific School of Harvard, where for the next two years he was a teacher of mathematics. Subsequently he became professor of physics at the Massachusetts Institute of Technology, and in 1876 he was appointed professor of astronomy and director of the Harvard College
observatory
 . In 1877 he decided to
devote one of the telescopes of the
observatory
  to stellar photometry, and after an exhaustive trial of various forms of photo-meters, he devised the meridian photometer (see PHOTOMETRY, STELLAR), which seemed to be free from most of the sources of error. With the first
instrument
  of this kind, having objectives of 1.5 inch aperture, he measured the brightness of 4260 stars, including all stars down to the 6th magnitude between the North Pole and -30 declination. With the object of reaching fainter stars, Professor Pickering constructed another
instrument
  of larger dimensions, and with this more than a million observations have been made. The first important
work
  undertaken with it was a revision of the magnitudes given in the Bonn Durchmusterung. On the completion of this, Professor Pickering decided to undertake the survey of the southern hemisphere. An expedition, under the direction of Prof. S. I. Bailey, was accordingly despatched (1889), and the meridian photometer erected successively in three different positions on the slopes of the Andes. The third of these was Arequipa, at which a permanent branch of the Harvard Observatory is now located. The .magnitudes of nearly 8000 southern stars were determined, including 1428 stars of the 6th magnitude and brighter. The instrument was then returned to
Cambridge
  (U.S.A.), where the survey extended so as to include all stars of magnitude 7.5 down to -40 declination, after which it was once more sent back to Arequipa. In 1886 the widow of
Henry
 
Draper
 , one of the pioneers of stellar spectroscopy, made a liberal provision for carrying on spectroscopic investigations at Harvard College in memory of her husband. With Professor Pickering's usual comprehensiveness, the inquiry was so arranged as to cover the whole sky; and with four telescopestwo at
Cambridge
  for the northern hemisphere, and two at Arequipa in Peru for the southernto which a fine 24-in. photographic telescope was afterwards added, no fewer than 75,000 photographs had been obtained up to the beginning of 1901. These investigations have yielded many important discoveries, not only of new stars, and of large numbers of variable stars, but also of a wholly new class of
double
  stars whose binary character is only revealed by peculiarities in their spectra. The important conclusion has been already derived that the
majority
  of the stars in the Milky Way belong to one
special
  type.


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