In the 17th century, Kepler proposed his ‘law of harmonies’ for planetary motion. This law suggested that the ratio of the square of the orbital period T to the cube of the mean radius R has the same value for all the planets that orbit the Sun.
Mathematically his ‘law of harmonies’ can be written
where K is a constant.
Kepler’s law of harmonies was derived later by Newton. Newton applied his law of gravitation to a planet moving in an approximately circular orbit around the Sun.
Determine a value for K by applying Newton’s law of gravitation to a planet of mass m moving in a circular orbit about the Sun.
mass of Sun = 1.99 × 1030 kg
K = .............................. s2 m–3
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