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Parallax is the apparent displacement of an object because of a change in the observer's point of view.
Another way to see how this effect works is to hold your hand out in front of you and look at it with your
left eye closed, then your right eye closed. Your hand will appear to move against the background.
This effect can be used to measure the distances to nearby stars. As the Earth orbits the Sun, a nearby
star
will appear to move against the more distant background stars. Astronomers can measure a star's position
once, and then again 6 months later and calculate the apparent change in position.
The star's apparent
motion is called stellar parallax.
Parallax angles of less than 0.01 arcsec are very difficult to measure from Earth because of the effects of
the Earth's atmosphere. This limits Earth based telescopes to measuring the distances to stars about 1/0.01
or 100 parsecs away. Space based telescopes can get accuracy to 0.001, which has increased the number of
stars whose distance could be measured with this method.
However, most stars even in our own galaxy are
much
further away than 1000 parsecs, since the Milky Way is about 30,000 parsecs across.