Stellar Physics Calculator
Complete stellar physics calculations. Analyze luminosity, temperature, nuclear fusion, stellar evolution, black body radiation, and stellar distances.
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How to Use This Calculator
- Follow the step-by-step wizard — complete each step before moving to the next. This guided approach ensures you provide all the necessary information in a logical order.
- Calculation Type — Calculation mode to use. Choose from: Luminosity & Temperature, Nuclear Fusion & Energy, Stellar Evolution, Black Body Radiation, Distances & Magnitudes. default: 0.
- Stellar Mass (M☉) — Mass in solar masses default: 1.
- Stellar Radius (R☉) — Radius in solar radii default: 1.
- Surface Temperature (K) — Effective surface temperature default: 5,778.
- Stellar Mass (M☉) — enter a numeric value. default: 1.
- Core Temperature (Million K) — Sun's core is 15.7 MK default: 15.7.
- Hydrogen Mass Fraction — Typical: 0.71 for solar composition default: 0.71.
- Helium Mass Fraction — Typical: 0.27 for solar composition default: 0.27.
- Initial Mass (M☉) — enter a numeric value. default: 1.
- Current Age (Billion Years) — Sun is 4.6 billion years old default: 4.6.
- Metallicity (Z/Z☉) — 1 = Solar, <1 = metal-poor, >1 = metal-rich default: 1.
- Temperature (K) — Temperature in the selected unit. default: 5,778.
- Radius (R☉) — Distance from center to edge. default: 1.
- Apparent Magnitude (m) — How bright star appears from Earth default: 0.
- Absolute Magnitude (M) — Brightness at 10 parsecs (Sun = 4.83) default: 4.83.
- Parallax (arcseconds) — Annual parallax shift (optional) default: 0.
- Distance (parsecs) — Known distance (optional) default: 0.
- Once all inputs are set, review your results in the Results panel. Here's what each output means:
- Luminosity (L☉) — shown as a numeric value. This is the primary result of this calculator.
- Absolute Magnitude — shown as a numeric value. This is the primary result of this calculator.
- Peak Wavelength (nm) — shown as a numeric value.
- Spectral Class — your calculated result.
- Luminosity Class — your calculated result.
- MS Lifetime (Gyr) — shown as a numeric value.
- Surface Gravity (g☉) — shown as a numeric value.
- Escape Velocity (km/s) — shown as a numeric value.
- H Burn Rate (× Sun) — shown as a numeric value.
- Fuel Remaining (Gyr) — shown as a numeric value.
- pp-Chain (%) — shown as a numeric value.
- CNO Cycle (%) — shown as a numeric value.
- Current Stage — your calculated result.
- Next Stage — your calculated result.
- Time to Next (Gyr) — shown as a numeric value.
- Final Remnant — your calculated result.
- Remnant Mass (M☉) — shown as a numeric value.
- Total Power (L☉) — shown as a numeric value.
- Dominant Color — your calculated result.
- UV Fraction (%) — shown as a percentage.
- Visible Fraction (%) — shown as a percentage.
- IR Fraction (%) — shown as a percentage.
- Distance (pc) — shown as a numeric value.
- Distance (ly) — shown as a numeric value.
- Distance Modulus — shown as a numeric value.
- Luminosity (L☉) — shown as a numeric value.
- Light Travel Time (yr) — shown as a numeric value.
- View the Stellar Comparison below for a visual breakdown of how the numbers relate to each other.
- Check the Stellar Properties for a detailed row-by-row breakdown. This is useful for spotting trends or finding values at specific points.
- Explore the related calculators below if you need deeper analysis or want to approach this topic from a different angle.
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Formula
L = 4πR²σT⁴ (Stefan-Boltzmann) | λ_peak = b/T (Wien's Law) | m - M = 5log₁₀(d) - 5Related Calculators
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