The Popular Science Monthly, September, 1900: Vol. 57, May, 1900 to October, 1900Various
Science
The Popular Science Monthly, September, 1900: Vol. 57, May, 1900 to October, 1900
Various
Science -- Periodicals; Technology -- Periodicals
A comparison of these numbers shows how much the result depends on the
special stars selected. By leaving out 26 stars the apex is changed by
5° in R. A., and 7° in declination.
It is to be remarked that the stars used by Boss are all contained in a
belt four degrees wide, extending from 1° to 5° north of the equator.
Dr. Oscar Stumpe, of Berlin, made a list of 996 stars having proper
motions between 16″ and 128″ per century. He divided them into three
groups, the first including those between 16″ and 32″; the second
between 32″ and 64″; the third between 64″ and 128″. The number of
stars in each group and the position of the apex derived from them are
as follows:
Gr. I, 551 stars; A = 287°.4; D = × 45°.0
II, 339 282°.2 43°.5
III, 106 280°.2 33°.5
Porter, of Cincinnati, made a determination from a yet larger list of
stars with results of the same general character.
These determinations have the advantage that the stars are scattered
over the entire heavens, the southern as well as the northern ones.
The difference of more than 10° between the position derived from
stars with the largest proper motions, and from the other stars, is
remarkable.
The present writer, in a determination of the precessional motion,
incidentally determined the solar motion from 2,527 stars contained in
Bradley’s Catalogue which had small proper motions, and from about 600
more having larger proper motions. Of the latter the declinations only
were used. The results were:
From small motions: A = 274°.2; D = × 31°.2
From large motions: 276°.9 31°.4
From all these results it would seem that the most likely apex of the
solar motion is toward the point in
Right Ascension, 280°
Declination, 38° north.
This point is situated in the constellation Lyra, about 2° from the
first magnitude star Vega. The uncertainty of the result is more than
this difference, four or five degrees at least. We may therefore state
the conclusion in this form:
_The apex of the solar motion is in the general direction of the
constellation Lyra, and probably very near the star Vega, the brightest
of that constellation._
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