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Calcimator

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
  1. 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.
  2. Calculation Type — Calculation mode to use. Choose from: Luminosity & Temperature, Nuclear Fusion & Energy, Stellar Evolution, Black Body Radiation, Distances & Magnitudes. default: 0.
  3. Stellar Mass (M☉) — Mass in solar masses default: 1.
  4. Stellar Radius (R☉) — Radius in solar radii default: 1.
  5. Surface Temperature (K) — Effective surface temperature default: 5,778.
  6. Stellar Mass (M☉) — enter a numeric value. default: 1.
  7. Core Temperature (Million K) — Sun's core is 15.7 MK default: 15.7.
  8. Hydrogen Mass Fraction — Typical: 0.71 for solar composition default: 0.71.
  9. Helium Mass Fraction — Typical: 0.27 for solar composition default: 0.27.
  10. Initial Mass (M☉) — enter a numeric value. default: 1.
  11. Current Age (Billion Years) — Sun is 4.6 billion years old default: 4.6.
  12. Metallicity (Z/Z☉) — 1 = Solar, <1 = metal-poor, >1 = metal-rich default: 1.
  13. Temperature (K) — Temperature in the selected unit. default: 5,778.
  14. Radius (R☉) — Distance from center to edge. default: 1.
  15. Apparent Magnitude (m) — How bright star appears from Earth default: 0.
  16. Absolute Magnitude (M) — Brightness at 10 parsecs (Sun = 4.83) default: 4.83.
  17. Parallax (arcseconds) — Annual parallax shift (optional) default: 0.
  18. Distance (parsecs) — Known distance (optional) default: 0.
  19. Once all inputs are set, review your results in the Results panel. Here's what each output means:
  20. Luminosity (L☉) — shown as a numeric value. This is the primary result of this calculator.
  21. Absolute Magnitude — shown as a numeric value. This is the primary result of this calculator.
  22. Peak Wavelength (nm) — shown as a numeric value.
  23. Spectral Class — your calculated result.
  24. Luminosity Class — your calculated result.
  25. MS Lifetime (Gyr) — shown as a numeric value.
  26. Surface Gravity (g☉) — shown as a numeric value.
  27. Escape Velocity (km/s) — shown as a numeric value.
  28. H Burn Rate (× Sun) — shown as a numeric value.
  29. Fuel Remaining (Gyr) — shown as a numeric value.
  30. pp-Chain (%) — shown as a numeric value.
  31. CNO Cycle (%) — shown as a numeric value.
  32. Current Stage — your calculated result.
  33. Next Stage — your calculated result.
  34. Time to Next (Gyr) — shown as a numeric value.
  35. Final Remnant — your calculated result.
  36. Remnant Mass (M☉) — shown as a numeric value.
  37. Total Power (L☉) — shown as a numeric value.
  38. Dominant Color — your calculated result.
  39. UV Fraction (%) — shown as a percentage.
  40. Visible Fraction (%) — shown as a percentage.
  41. IR Fraction (%) — shown as a percentage.
  42. Distance (pc) — shown as a numeric value.
  43. Distance (ly) — shown as a numeric value.
  44. Distance Modulus — shown as a numeric value.
  45. Luminosity (L☉) — shown as a numeric value.
  46. Light Travel Time (yr) — shown as a numeric value.
  47. View the Stellar Comparison below for a visual breakdown of how the numbers relate to each other.
  48. Check the Stellar Properties for a detailed row-by-row breakdown. This is useful for spotting trends or finding values at specific points.
  49. 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) - 5

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