Stellar parallax
What is stellar parallax? Convert a parallax angle to distance with d = 1/p: 0.1″ → 10 parsecs (32.6 light-years). Interactive diagram and worked examples.
Your experiment
How it works
As Earth moves around the Sun, a nearby star appears to shift against distant background stars. The annual parallax is half of the total angular shift between opposite points in Earth’s orbit.
What Is Stellar Parallax? Formula & Diagram ↗About this model
The standard small-angle parsec relation with exact input. The diagram exaggerates angles and compresses distances. Real measurements include uncertainty and corrections.
Key formulas
| Quantity | Formula | Note or example |
|---|---|---|
| Parallax distance | d (parsecs) = 1 ÷ p (arcseconds) | p is the annual parallax |
| Parsec in light-years | 1 pc ≈ 3.26 ly | |
| Parsec in AU | 1 pc ≈ 206,265 AU |
Worked examples
Each row uses one of this lab’s presets and the same model as the interactive tool.
| Example | Distance | Light travel | Parallax |
|---|---|---|---|
| Proxima Centauri | 1.3 pc | 4.25 years | 0.768″ |
| Ten parsecs | 10 pc | 32.62 years | 0.1″ |
| One kiloparsec | 1,000 pc | 3,261.56 years | 0.001″ |
Stellar parallax: common questions
What is a parsec?
A parsec is the distance corresponding to one arcsecond of annual parallax, approximately 3.26 light-years.
Why are distant stars harder to measure?
Their parallax angles are smaller, so a fixed angular uncertainty represents a larger fraction of the measurement.
What is stellar parallax?
Stellar parallax is the small apparent shift of a nearby star against much more distant stars as Earth orbits the Sun. The annual parallax angle p is half the total shift; 1 ÷ p gives the distance in parsecs.
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