Stellar Parallax Distance Calculator
Estimate the distance to a star based on its parallax angle in arcseconds.
Formulas Used
The distance to a star is calculated using the parallax angle, with results provided in parsecs and light-years.
- Distance in Parsecs:
\[ d = \frac{1}{\text{parallax}} \]
Calculates the distance in parsecs, where parallax is in arcseconds.
- Distance in Light-Years:
\[ d_{\text{ly}} = d \times 3.26156 \]
Converts parsecs to light-years using the conversion factor 1 parsec ≈ 3.26156 light-years.
Example Calculations
Example 1: Nearby Star
Input: Parallax Angle = 0.2 arcseconds
Calculations:
- Distance in Parsecs: \[ \frac{1}{0.2} = 5 \text{ parsecs} \]
- Distance in Light-Years: \[ 5 \times 3.26156 \approx 16.31 \text{ light-years} \]
Result: Distance: 5 parsecs (16.31 light-years)
Example 2: Distant Star
Input: Parallax Angle = 0.01 arcseconds
Calculations:
- Distance in Parsecs: \[ \frac{1}{0.01} = 100 \text{ parsecs} \]
- Distance in Light-Years: \[ 100 \times 3.26156 \approx 326.16 \text{ light-years} \]
Result: Distance: 100 parsecs (326.16 light-years)
Example 3: Very Close Star
Input: Parallax Angle = 0.768 arcseconds
Calculations:
- Distance in Parsecs: \[ \frac{1}{0.768} \approx 1.30 \text{ parsecs} \]
- Distance in Light-Years: \[ 1.30 \times 3.26156 \approx 4.24 \text{ light-years} \]
Result: Distance: 1.30 parsecs (4.24 light-years, similar to Proxima Centauri)
How to Use the Calculator
Follow these steps to estimate the distance to a star:
- Enter Parallax Angle: Input the star’s parallax angle in arcseconds (e.g., 0.1 for a star at 10 parsecs).
- Calculate: Click “Calculate Distance” to see the result.
- Interpret Result: The result shows the distance in parsecs and light-years. If you see “Please fill in all fields,” ensure the parallax angle is provided and positive.
- Share or Embed: Use the share buttons to post results on social media, copy the result, or get an embed code for the calculator.
Note: This calculator assumes accurate parallax measurements. Actual measurements may include observational errors, and distances are approximate.