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Luminosity & the Inverse-Square Law

Lesson 6 of 818 minLab

This lesson is part of the course

In this lesson

You compute the Sun's power output from its size and temperature, the sunlight each planet receives and where other stars would warm a planet like the Sun warms Earth.

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Lessons in this course

  1. Cosmic Units: AU, Light-Years & ParsecsLab12 min Locked
  2. Kepler's Third Law: Periods, Orbits & a Log-Log PlotLab15 min Locked
  3. Orbital Speed, Escape Velocity & Weighing the SunLab15 min Locked
  4. Parallax: Distances to the Nearest StarsLab12 min Locked
  5. Apparent vs Absolute Magnitude & the Distance ModulusLab15 min Locked
  6. Luminosity & the Inverse-Square LawLab18 min Locked
  7. Wien's Law: Star Temperature, Colour & Spectral ClassLab15 min Locked
  8. Hubble's Law: Fitting H₀ & the Age Scale of the UniverseLab18 min Locked