Proper motion is apparent movement of an astronomical object in the plane of the sky, usually measured in arcseconds per year. You need to know the distance to translate this into km/second. Proper motion is in a plane orthogonal to DopplerVelocity.

-- AnitaRichards - 24 Apr 2003

Topic revision: r1 - 2003-04-24 - 18:58:22 - AnitaRichards
 
AstroGrid Service Click here for the
AstroGrid Service Web
This is the AstroGrid
Development Wiki

This site is powered by the TWiki collaboration platformCopyright © by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback