Parallax is the tiny apparent shift in a nearby star's position when viewed from opposite sides of Earth's orbit.
Parallax is the tiny apparent shift in a nearby star's position when viewed from opposite sides of Earth's orbit. The smaller that shift, the farther away the star is — giving astronomers a direct, geometric way to measure stellar distances.
Proxima Centauri has a parallax of about 0.769 arcseconds. Distance = 1/0.769 ≈ 1.30 pc ≈ 4.24 light-years — matching its known distance as the nearest star to the Sun.
The apparent shift in a nearby star's position observed from two points in Earth's orbit.
Distance in parsecs = 1 ÷ parallax angle in arcseconds.
The angle becomes too small to measure accurately for very distant stars.