Question

According to Kepler's third law T square is directly proportional to r raise to n, where n is equal to? *​

Answer 1

Answer:

What's inside the brackets is just a number. The rest tells a simple message--T2 is proportional to r3, the orbital period squared is proportional to the distance cubes. This is Kepler's 3rd law, for the special case of circular orbits around Earth

Step-by-step explanation:

Answer 2

Answer:

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 than as per Newton's law of gravitation force of attraction between them is

F= r 2GMm

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