The planets move on ellipses, and a planet moves faster when it is near the Sun. Kepler found these rules from many years of observations, and Newton explained them with one law. In this course we study the three laws of Kepler, we write Newton's law of gravitation and find the force between two bodies, and we find how the acceleration due to gravity changes with height, with depth and with the turning of the Earth.
3 lessons, about 1 h 15 min3 simulations12 problems6 practice questionsPython in every lesson
Kepler found three laws in Tycho Brahe's measurements. The planets move in ellipses, with the Sun at one focus. The line from the Sun to a planet sweeps out equal areas in equal times, so a planet is fastest when nearest. The square of a planet's year is proportional to the cube of its mean distance: .
Every two bodies attract each other along the line joining them with , where . The pulls on the two bodies are equal and opposite. A uniform sphere pulls as if all its mass were at its centre. The force is tiny between everyday objects and huge between planets.
At the Earth's surface, , about . Above the surface it falls as : for small . Below the surface of a uniform Earth it falls in a straight line, , to zero at the centre. The Earth's spin and bulge make a little smaller at the equator.
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