Kepler’s Third Law Calculator

Kepler’s Third Law, formulated by Johannes Kepler in the early 17th century, describes the relationship between the orbital period and the semi-major axis of a planet’s orbit around the Sun. This law is fundamental in understanding the dynamics of celestial bodies within our solar system and beyond.

Where:

  • is the orbital period of the planet (time taken to complete one orbit).
  • is the gravitational constant.
  • is the mass of the central body (usually the Sun).
  • is the average distance between the planet and the Sun.

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