Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
The catalogues of variable stars now contain many thousands of these
objects. They are often designated by the letters R, S, T, and so on,
followed by the genitive form of the name of the constellation wherein
they are found. Most of the recently found variables have a range of
less than one magnitude. They are so distributed as to be most numerous
in a zone inclined about 18 degrees to the celestial equator, and split
in two near where the cleft in the Galaxy is located. Nearly all the
temporary stars are in this duplex region. Bailey of Harvard a quarter
century ago began the investigation of variables in close star clusters,
where they are very abundant, with marked changes of magnitude within
only a few hours.
Many amateur astronomers afford very great assistance to the
professional investigator of variable stars by their cooperation in
observing these interesting bodies, in particular the American
Association of Observers of Variable Stars, organized and directed by
William Tyler Olcott.
For a high degree of accuracy in determining stellar magnitudes the
photo-electric cell is unsurpassed. Stebbins of Urbana has been very
successful in its application and he discovered the secondary minimum of
Algol with the selenium cell. His most recent work was done with a
potassium cell with walls of fused quartz, perfected after many trial
attempts. The stars he has recently investigated are Lambda Tauri,
and Pi Five Orionis. Combining results with those reached by the
spectroscope, the masses of the two component stars of the former are
2.5 and 1.0 that of the sun, and the radii are 4.8 and 3.6 times the
sun's.
Russell of Princeton thinks it probable that similar causes are at work
in all these variables. In the case of the typical Novæ there is
evidence that when the outburst takes place a shell of incandescent gas
is actually ejected by the star at a very high velocity. What may be the
forces that cause such an explosion can only be guessed. Repeated
outbursts have not, in the case of T Pyxidis, destroyed the star,
because it has gone through this process three times in the past thirty
years. Russell inclines to regard it as a standard process occurring
somewhere in the stellar universe probably as often as once a year.
Public-domain text, read in full here on John Shaqi.
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