Solving and verifying Kepler’s third law in circular orbits
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Solving and verifying Kepler’s third law in circular orbits
1 month ago
MSNDot Physics
Kepler's third law states that square of period of revolution (T) of a planet around the sun, is proportional to third power of average distance r between sun and planet i.e. T^2 = Kr^3 here K is constant. If the masses of sun and planet are M and m respectively then as per Newton's law of gravitation force of attraction between them is F = GMm2 , here G is gravitational constant. The relation between G and K is described as
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