Proper Motion
Encyclopedia article; The Columbia Encyclopedia, Sixth Edition, 2004.
52323 pgs.

Proper Motion
Encyclopedia article; The Columbia Encyclopedia, Sixth Edition, 2004
Proper Motion
Encyclopedia article; The Columbia Encyclopedia, Sixth Edition, 2004
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PROPER MOTION in astronomy, apparent movement of a star on the
celestial sphere, usually measured as seconds of arc per year; it is due both to the actual relative motions of the sun and the star through space. Proper motion reflects only transverse motion, i.e., the component of motion across the line of sight to the star; it does not include the component of motion toward or away from the sun. The most distant stars show the least proper motion. Barnard's Star, one of the closest stars, has the largest measured proper motion, 10.27 sec of arc per year. The average proper motion of the stars that can be seen with the naked eye is 0.1″ per year. ____________________The Columbia Encyclopedia, Sixth Edition Copyright© 2004, Columbia University Press. Licensed from Lernout & Hauspie Speech Products N.V. All rights reserved. -38855- | |
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Publication Information: Encyclopedia Article Title: Proper Motion. Encyclopedia Title: The Columbia Encyclopedia, Sixth Edition. Publisher: Columbia University Press. Place of Publication: New York. Publication Year: 2004.
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