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The gravitational force of a star on an orbiting planet 1 is f1. planet 2, which is three times as massive as planet 1 and orbits at twice the distance from the star, experiences gravitational force f2. part a what is the ratio f2f1? you can ignore the gravitational force between the two planets.

User Pratham
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Let us consider two bodies having masses m and m' respectively.

Let they are separated by a distance of r from each other.

As per the Newtons law of gravitation ,the gravitational force between two bodies is given as -
F = G(mm')/(r^(2) ) where G is the gravitational force constant.

From the above we see that F ∝ mm' and
F\alpha (1)/(r^(2) )

Let the orbital radius of planet A is
r_(1) = r and mass of planet is
m_(1).

Let the mass of central star is m .

Hence the gravitational force for planet A is
f_(1) =G (m_(1)*m )/(r^(2) )

For planet B the orbital radius
r_(2) =2r_(1) and mass
m_(2) = 3 m_(1)

Hence the gravitational force
f_(2) =G(m m_(2) )/(r^(2) )


f_(2) =G(m*3m_(1) )/([2r_(1)] ^(2) )


= (3)/(4) G(mm_(1) )/(r_(1) ^(2) )

Hence the ratio is
(f_(2) )/(f_(1) ) = \frac{(3)/(4)G mm_{1/r_(1) ^2}  }{Gmm_(1)/r_(1) ^2 }


=(3)/(4) [ ans]