Man's Place in the Universe: A Study of the Results of Scientific Research in Relation to the Unity or Plurality of Worlds, 3rd EditionWallace, Alfred Russel
Science
Man's Place in the Universe: A Study of the Results of Scientific Research in Relation to the Unity or Plurality of Worlds, 3rd Edition
Wallace, Alfred Russel
Life; Plurality of worlds; Stars
Zones of Galactic Average number of Star
North Polar Distance. per Field of 15'.
0° to 15° 4.32
15° to 30° 5.42
30° to 45° 8.21
45° to 60° 13.61
60° to 75° 24.09
75° to 90° 53.43
Zones of Galactic Average number of Stars
South Polar Distance. per Field of 15'.
0° to 15° 6.05
15° to 30° 6.62
30° to 45° 9.08
45° to 60° 13.49
60° to 75° 26.29
75° to 90° 59.06
In these tables the Milky Way itself is taken as occupying two zones of 15°
each, instead of one of 20° as in Professor Newcomb's tables, so that the
excess in the number of stars over the other zones is not so large. They
show also a slight preponderance in all the zones of the southern
hemisphere, but this is not great, and may probably be due to the clearer
atmosphere of the Cape of Good Hope as compared with that of England.
[Illustration: DIAGRAM OF STAR-DENSITY. From Table in Sir J. Herschel's
_Outlines of Astronomy_ (10th ed., pp. 577-578).]
It need only be noted here that this diagram shows the same general
features as those already given, of a continuous increase of star-density
from the poles of the Galaxy, but more rapidly as the Galaxy itself is
more nearly approached. This fact must, therefore, be accepted as
indisputable.
CLUSTERS AND NEBULÆ IN RELATION TO THE GALAXY
An important factor in the structure of the heavens is afforded by the
distribution of the two classes of objects known as clusters and nebulæ.
Although we can form an almost continuous series from double stars which
revolve round their common centre of gravity, through triple and quadruple
stars, to groups and aggregations of indefinite extent--of which the
Pleiades form a good example, since the six stars visible to the naked eye
are increased to hundreds by high telescopic powers, while photographs with
three hours' exposure show more than 2000 stars--yet none of these
correspond to the large class known as clusters, whether globular or
irregular, which are very numerous, about 600 having been recorded by Sir
John Herschel more than fifty years ago. Many of these are among the most
beautiful and striking objects in the heavens even with a very small
telescope or good opera-glass. Such is the luminous spot called Praesepe,
or the Beehive in the constellation Cancer, and another in the sword handle
of Perseus.
Public-domain text, read in full here on John Shaqi.
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