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proper motion

(PM)
(apparent motion in relation to the position of the Sun)

Proper motion (PM) of a star is its change in angular position over time, corrected for the Earth's orbit, measured in angle (e.g., arcseconds) per year. If you could measure the position of an object at two instances precisely one year apart, the angle in arcseconds between the two measured positions would be its proper motion. Proper motion is an indication of relative motion between the star and the Sun, but does not fully characterize it, which also requires knowing the distance to the star and the star's radial velocity.

Common proper motion is such motion when it is shared by two stars, evidence they are a binary star.


(astrometry,measure)
http://en.wikipedia.org/wiki/Proper_motion
http://www.astronomy.ohio-state.edu/~pogge/Ast162/Unit1/motions.html

Referenced by:
Astrographic Catalog (AC)
baseline
Bruce Proper Motion Survey (BPM)
double star
epoch
fixed star
Frank Ross's Catalog (Ross)
G239-25
Gaia
Herschel Double Star Catalog (H)
epoch J2000.0
Kapteyn's Star
Lacaille 9352
Luyten Half-second Catalog (LHS)
Lowell Proper Motion Survey (G)
Luyten Palomar Survey (LP)
Lépine Shara Proper Motion catalog (LSPM)
Luyten Two-Tenths Arcsecond Catalog (LTT)
Max Wolf's catalog of stars with proper motion
moving-cluster method
position angle
PPM Star Catalogue
rare designator prefixes
SIMP
SuperCOSMOS Sky Survey (SSS)

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