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Q.

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 the sun and planet, i.e. T2 = Kr3, here K is constant. If the masses of the sun and planet are M and m respectively, then as per Newton's law of gravitational force of attraction between them is  F=GMmr2, here G is gravitational constant. The relation between G and K is described as  [CBSE AIPMT 2015]

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a

GK=4π2

b

GMK=4π2

c

K = G

d

K=I / G

answer is B.

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Detailed Solution

The gravitational force of attraction between the planet and sun provides the centripetal force,

i.e.,       GMmr2=mv2rv=GMr

The time period of planet will be

T=2πrv

  T2=4π2r2GMr=4π2r3GM                                            …(i)

Also, from the Kepler's third law,   T2=Kr3                        …(ii)

From Eqs. (i) and (ii), we get

4π2r3GM=Kr3GMK=4π2

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