Star Distance Calculator

Measuring the Stars With Nothing but a Triangle

Stellar parallax is the oldest reliable method for measuring distance beyond the solar system, and it still underpins modern astrometry missions like Gaia. The idea is pure geometry: observe a nearby star from two points six months apart — opposite sides of Earth's orbit — and measure how far it appears to shift against the distant background stars. That tiny shift, the parallax angle, shrinks as distance grows, which is exactly what makes it a distance ruler.

The Formula

Distance (parsecs) = 1 ÷ Parallax (arcseconds)

This is in fact the definition of the parsec itself: a star with a parallax of exactly 1 arcsecond sits, by definition, 1 parsec away. Every other distance falls out of that same inverse relationship — halve the parallax angle and the star is twice as far away.

Where Parallax Distance Matters

  • Calibrating the cosmic distance ladder — parallax is the only truly direct geometric distance measurement in astronomy; every more distant method (standard candles, redshift) is ultimately calibrated against parallax measurements of nearby stars.
  • Stellar catalogs — the Gaia mission has measured parallax for over a billion stars, and converting those raw angles to distances in parsecs or light-years is a routine step in using that data.
  • Nearest-neighbor astronomy — Proxima Centauri, the closest star to the Sun, was itself identified and confirmed largely through its comparatively large parallax angle.

Parallax Angle vs. Distance

Distance computed directly from parallax angle using Distance = 1 ÷ parallax
Parallax angleDistance (parsecs)Distance (light-years)
0.7687″ (Proxima Centauri's actual parallax)1.3009 pc4.243 ly
0.5″2.0000 pc6.523 ly
0.3″3.3333 pc10.872 ly
0.1″10.0000 pc32.616 ly
0.05″20.0000 pc65.231 ly
0.01″100.0000 pc326.156 ly
0.001″1,000.0000 pc3,261.564 ly

Proxima Centauri's parallax (0.7687 arcseconds) is a well-established published measurement, included here as a real-world reference point; all distances are computed directly from the calculator's own formula.

How to Use This Calculator

  1. Enter the star's measured parallax angle in arcseconds.
  2. Select Calculate to get the distance in both parsecs and light-years.

Related Calculations

Once you have a distance, the Light Year Calculator converts it into kilometers, miles, or astronomical units for easier comparison.