Physique
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Parallax Calculator.
Estimate distance from annual stellar parallax in arcseconds.
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Use Cases
Astronomy Education
Helps students and enthusiasts understand how astronomers measure stellar distances using parallax.
Example: Input a parallax of 0.5 arcsec to see the distance is 2 parsecs.
Quick Distance Estimation
Provides a fast way to convert a measured parallax angle into a distance without manual calculation.
Example: For a parallax of 0.05 arcsec, the distance is 20 parsecs.
Frequently Asked Questions
- What is the parallax formula used in this calculator?
- The calculator uses the formula distance (in parsecs) = 1 / parallax angle (in arcseconds). For example, a parallax of 0.1 arcsec gives a distance of 10 parsecs.
- Why is the distance in parsecs?
- The parsec is defined as the distance at which one astronomical unit subtends an angle of one arcsecond. Using the inverse relationship, a parallax of 1 arcsec equals 1 parsec, making the calculation straightforward.
- Can I use this for any star?
- Yes, as long as you have the annual parallax angle in arcseconds. This method is most accurate for nearby stars; for distant stars, the parallax is very small and harder to measure precisely.
Tips & Common Mistakes
Tips
- Ensure the parallax angle is in arcseconds, not degrees or radians.
- Use precise measurements; small errors in parallax lead to large errors in distance.
- For very small parallax values (e.g., <0.01 arcsec), the distance is large and may be less reliable.
- Remember that 1 parsec ≈ 3.26 light-years if you need to convert to light-years.
Common Mistakes to Avoid
- Using the parallax angle in degrees instead of arcseconds.
- Forgetting that the formula is inverse: a larger parallax means a smaller distance.
- Assuming the result is in light-years when it is in parsecs.
Last updated: August 13, 2026