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.
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.
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; as, the
annual parallax of a fixed star. -- 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, 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.
Hear it pronounced