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 problem of spectroscopic determinations of luminosity and parallax
has been investigated at Mount Wilson with great thoroughness from all
sides, the separate investigations checking each other. A definitive
scale for the spectroscopic determination of absolute magnitudes has now
been established, and the parallaxes and absolute magnitudes have
already been derived for about 1,800 stars.
CHAPTER XLIX
THE NEAREST STARS
Of especial interest are the few stars that we know are the nearest to
us, and the following table includes all those whose parallax is 0".20
or greater. There are nineteen in all and nearly half of them are binary
systems. The radial motions given are relative to the sun. The
transverse velocities are formed by using the measured parallaxes to
transform proper motions into linear measures. They are given by
Eddington in his "Stellar Movements":
Column Key
====================
A) Magnitude
B) Parallax in Seconds of Arc
C) Proper Motion in Seconds of Arc
D) Linear Velocity Km. per sec.
E) Radial Velocity Km. per sec.
F) Spectral Type
G) Luminosity (Sun=1)
H) Star Stream
====================================================================
Star's Name | A | B | C | D | E | F | G | H
---------------+-----+------+------+-----+-----+------+-------+-----
Groombridge 34 | 8.2 | 0.28 | 2.85 | 48 | .. | Ma | 0.010 | I
Eta Cassiop | 3.6 | 0.20 | 1.25 | 30 | +10 | F8 | 1.4 | I
Tau Ceti | 3.6 | 0.33 | 1.93 | 28 | -16 | K | 0.50 | II
Epsilon Erid | 3.3 | 0.31 | 1.00 | 15 | +16 | K | 0.79 | II
CZ 5h 243 | 8.3 | 0.32 | 8.70 | 129 |+242 | G-K | 0.007 | II
Sirius |-1.6 | 0.38 | 1.32 | 16 | -7 | A |48.0 | II
Procyon | 0.5 | 0.32 | 1.25 | 19 | -3 | F5 | 9.7 | I ?
Lal. 21185 | 7.6 | 0.40 | 4.77 | 57 | .. | Ma | 0.009 | II
Lal. 21258 | 8.9 | 0.20 | 4.46 | 106 | .. | Ma | 0.011 | I
OA (N) 11677 | 9.2 | 0.20 | 3.03 | 72 | .. | .. | 0.008 | I
Alpha Centauri | 0.3 | 0.76 | 3.66 | 23 | -22 | G,K5 |{2.0 | I
| | | | | | |{0.6 |
OA (N) 17415 | 9.3 | 0.27 | 1.31 | 23 | .. | F | 0.004 | II
Pos. Med. 2164 | 8.8 | 0.29 | 2.28 | 37 | .. | K | 0.006 | I
Sigma Draco | 4.8 | 0.20 | 1.84 | 43 | +25 | K | 0.5 | II
Alpha Aquilæ | 0.9 | 0.24 | 0.65 | 13 | -33 | A5 |12.3 | I
61 Cygni | 5.6 | 0.31 | 5.25 | 80 | -39 | K5 | 0.10 | I
Epsilon Indi | 4.7 | 0.28 | 4.67 | 79 | -62 | K5 | 0.25 | I
Krüger 60 | 9.2 | 0.26 | 0.92 | 17 | .. | .. | 0.005 | II
Lacaille 9352 | 7.4 | 0.29 | 7.02 | 115 | +12 | Ma | 0.019 | I
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