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Optical parallax (gcide) | Parallax \Par"al*lax\, n. [Gr. ? alternation, the mutual
    inclination of two lines forming an angle, fr. ? to change a
    little, go aside, deviate; para` beside, beyond + ? to
    change: cf. F. parallaxe. Cf. Parallel.]
    1. The apparent displacement, or difference of position, of
       an object, as seen from two different stations, or points
       of view.
       [1913 Webster]
 
    2. (Astron.) The apparent difference in position of a body
       (as the sun, or a star) as seen from some point on the
       earth's surface, and as seen from some other conventional
       point, as the earth's center or the sun.
       [1913 Webster]
 
    3. (Astron.) The annual parallax. See annual parallax,
       below.
       [PJC]
 
    Annual parallax, the greatest value of the heliocentric
       parallax, or the greatest annual apparent change of place
       of a body as seen from the earth and sun; it is equivalent
       to the parallax of an astronomical object which would be
       observed by taking observations of the object at two
       different points one astronomical unit (the distance of
       the Earth from the sun) apart, if the line joining the two
       observing points is perpendicular to the direction to the
       observed object; as, the annual parallax of a fixed star.
       The distance of an astronomical object from the Earth is
       inversely proportional to the annual parallax. A star
       which has an annual parallax of one second of an arc is
       considered to be one parsec (3.26 light years) distant
       from the earth; a star with an annual parallax of
       one-hundredth second of an arc is 326 light years distant.
       See parsec in the vocabulary, and stellar parallax,
       below.
 
    Binocular parallax, the apparent difference in position of
       an object as seen separately by one eye, and then by the
       other, the head remaining unmoved.
 
    Diurnal parallax or Geocentric parallax, the parallax of
       a body with reference to the earth's center. This is the
       kind of parallax that is generally understood when the
       term is used without qualification.
 
    Heliocentric parallax, the parallax of a body with
       reference to the sun, or the angle subtended at the body
       by lines drawn from it to the earth and sun; as, the
       heliocentric parallax of a planet.
 
    Horizontal parallax, the geocentric parallx of a heavenly
       body when in the horizon, or the angle subtended at the
       body by the earth's radius.
 
    Optical parallax, the apparent displacement in position
       undergone by an object when viewed by either eye singly.
       --Brande & C.
 
    Parallax of the cross wires (of an optical instrument),
       their apparent displacement when the eye changes its
       position, caused by their not being exactly in the focus
       of the object glass.
 
    Stellar parallax, the annual parallax of a fixed star.
       [1913 Webster] |  
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