Friday, March 25, 2005

Proper Motion

In astronomy, the apparent motion of a star across the celestial sphere at right angles to the observer's line of sight; any radial motion (toward or away from the Sun) is not included. Proper motion is generally measured in seconds of arc per year; the largest known is that of Barnard's star in the constellation Ophiuchus, about 10² yearly. The English astronomer Edmond

0 Comments:

Post a Comment

<< Home