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Kepler’s Laws of Orbits

Planets travel around the Sun along ellipses, with the Sun at one focus. A planet sweeps out equal areas in equal times, and the square of its orbital period grows in proportion to the cube of its average distance from the Sun.

In the picture

  1. The Sun: one focus of the elliptical orbit
  2. The large bright oval: the planet’s closed elliptical path around the Sun
  3. The short wide wedge: the area swept close to the Sun in a fixed time
  4. The long narrow wedge: the same area swept farther from the Sun in the same time
  5. The smaller dotted oval: a smaller orbit with a shorter period, where T² is proportional to a³

Examples

  • A comet speeds up as it swings near the Sun and slows down as it moves far away.
  • Outer planets such as Neptune take much longer to orbit the Sun than inner planets such as Mercury.

Quiz: Kepler’s Laws of Orbits (Age 18)

  1. According to Kepler, what shape do planetary orbits around the Sun have?

    • Ellipses with the Sun at one focus
    • Perfect circles centered on the Sun
    • Ellipses with the Sun at the center
  2. What does the equal-area law say about a planet’s motion?

    • It moves at the same speed at every point in its orbit
    • It sweeps out a larger area when it is farther from the Sun
    • It sweeps out equal areas in equal times
  3. How does Kepler’s third law relate orbital period T to average distance a from the Sun?

    • T² is proportional to a²
    • T² is proportional to a³
    • T is proportional to a

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Physics, Age 18