Parallax is the angle between the apparent location of an object as seen from two different places. It is used to measure their distance to stars (stellar parallax). If a very small angle can be measured accurately, a distance to a nearby star can be determined.
For measuring distances to a star, the parallax used is the angle between viewing the star from Earth at two times, half a year apart, when the positions of the Earth differ by 2 AU (the baseline). The angle cited as parallax (parallax angle) is typically half this, the angle from two positions 1 AU apart, e.g., from the Sun and the Earth. A parsec is the distance of a star with this (1 AU) parallax angle of 1 arcsecond. Typical "rough" capabilities of telescopes:
|Ground-based telescope without adaptive optics||1 arcsecond||1 pc|
|With adoptive optics||50 milliarcseconds||20 pc|
|HST||50 milliarcseconds||20 pc|
|radio interferometer||5 milliarcseconds||200 pc|
|very-long-baseline interferometry (8000 km baseline)||1 milliarcsecond||1 kpc|
Secular parallax consists of using the Sun's motion to gain a longer baseline, but the fact that the target star also has such a motion limits the information that can be gained.