Pleasures of the telescope: An Illustrated Guide for Amateur Astronomers and a Popular Description of the Chief Wonders of the Heavens for General ReadersServiss, Garrett Putman
Science
Pleasures of the telescope: An Illustrated Guide for Amateur Astronomers and a Popular Description of the Chief Wonders of the Heavens for General Readers
The most beautiful double star in Cetus is gamma, magnitudes three and
seven, distance 3", p. 288 deg.; hues, straw-color and blue. The leading
star alpha, of magnitude two and a half, has a distant blue companion
three magnitudes fainter, and between them are two minute stars, the
southernmost of which is a double, magnitudes both eleven, distance 10",
p. 225 deg..
The variable S ranges between magnitudes seven and twelve in a somewhat
irregular period of about eleven months, while R ranges between the
seventh and the thirteenth magnitudes in a period of one hundred and
sixty-seven days.
[Illustration: MAP NO. 21.]
The constellation Eridanus, represented in map No. 21, contains a few
fine double stars, one of the most interesting of which is 12, a rather
close binary. The magnitudes are four and eight, distance 2", p. 327 deg..
We shall take the five-inch for this, and a steady atmosphere and sharp
seeing will be necessary on account of the wide difference in the
brightness of the component stars. Amateurs frequently fail to make due
allowance for the effect of such difference. When the limit of
separating power for a telescope of a particular aperture is set at 1"
or 2", as the case may be, it is assumed that the stars composing the
doubles on which the test is made shall be of nearly the same magnitude,
or at least that they shall not differ by more than one or two
magnitudes at the most. The stray light surrounding a comparatively
bright star tends to conceal a faint companion, although the telescope
may perfectly separate them so far as the stellar disks are concerned.
Then, too, I have observed in my own experience that a very faint and
close double is more difficult than a brighter pair not more widely
separated, usually on account of the defect of light, and this is true
even when the components of the faint double are of equal magnitude.
Sigma 470, otherwise known as 32 Eridani, is a superb object on account
of the colors of its components, the larger star being a rich topaz and
the smaller an ultramarine; while the difference in magnitude is not as
great as in many of the colored doubles. The magnitudes are five and
seven, distance 6.7", p. 348 deg.. The star gamma, of magnitude two and a
half, has a tenth-magnitude companion, distant 51", p. 238 deg.. Sigma 516,
also called 39 Eridani, consists of two stars of magnitudes six and
nine, distance 6.4", p. 150 deg.; colors, yellow and blue. The supposed
binary character of this star has not yet been established.
Public-domain text, read in full here on John Shaqi.
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