Mass of the Sun, Ms = 2 × 1030 kg
Mass of the Earth, Me = 6 × 1024 kg
Orbital radius, r = 1.5 × 1011 m
Mass of the rocket = m

Let x be the distance from the centre of the Earth where the gravitational force acting on satellite P becomes zero.
From Newton’s law of gravitation, we can equate gravitational forces acting on satellite P under the influence of the Sun and the Earth as:
