Kepler’s Three Laws of Planetary Motion

keplerThe laws were formulated between 1609 to 16l9, and are (as usually stated):

  • Planets move around the Sun in ellipses, with the Sun at one focus
  • The line connecting the Sun to a planet sweeps equal areas in equal times.
  • The square of the orbital period of a planet is proportional to the cube (3rd power) of the mean distance from the Sun in (or in other words–of the"semi-major axis" of the ellipse, half the sum of smallest and greatest distance from the Sun)

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