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proper motion | ||||
subject | fact |
proper motion | has definition Apparent angular rate of motion of a star across the line of sight on the celestial sphere. | |
has definition The apparent movement of a star, year after year, caused by the star's velocity across the line of sight. If the star's distance is known, this velocity-called the tangential velocity, can be computed. The star with the largest proper motion is Barnard's Star, whose proper motion is 10.3 arc-seconds per year. | ||
has definition The projection onto the celestial sphere of the space motion of a star relative to the solar system; thus the transverse component of the space motion of a star with respect to the solar system. Proper motion is usually tabulated in star catalogs as changes in right ascension and declination per year or century. | ||
is a kind of motion | ||
physical process | has domain physics |
Kinds of proper motion :