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A body of mass 2M splits into four masses {m,m,M-m,M-m}, which are rearranged to form a square as shown in the figure. The ratio of Mm for which, the gravitational potential energy of the system becomes maximum is x : 1. The value of x is ________.

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Important Questions on Gravitation

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JEE Main
IMPORTANT
A mass of 50 kg is placed at the center of a uniform spherical shell of mass 100 kg and radius 50 m. If the gravitational potential at a point, 25 m from the center is V kg m-1. The value of V is:
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The masses and radii of the earth and moon are M1, R1 and M2, R2 respectively. Their centres are at a distance r apart. Find the minimum escape velocity for a particle of mass m  to be projected from the middle of these two masses :
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If RE be the radius of Earth, then the ratio between the acceleration due to gravity at a depth r below and a height r above the earth surface is:
(Given : r<RE)
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Four particles each of mass M, move along a circle of radius R under the action of their mutual gravitational attraction as shown in figure. The speed of each particle is :

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Two satellites revolve around a planet in coplanar circular orbits in anticlockwise direction. Their period of revolutions are 1 hour and 8 hours respectively. The radius of the orbit of nearer satellite is 2×103 km. The angular speed of the farther satellite as observed from the nearer satellite at the instant when both the satellites are closest is πxradh-1, where x is _______.
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A person whose mass is 100 kg travels from Earth to Mars in a spaceship. Neglect all other objects in sky and take acceleration due to gravity on the
surface of the Earth and Mars as 10 m s-2 and 4 m s-2, respectively. Identify from the below figures, the curve that fits best for the weight of the passenger as a function of time.

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IMPORTANT
A satellite is launched into a circular orbit of radius R around earth, while a second satellite is launched into a circular orbit of radius 1.02 R. The percentage difference in the time periods of the two satellites is:
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JEE Main
IMPORTANT
Consider a binary star system of star A and star B with masses mA and mB revolving in a circular orbit of radii rA and rB, respectively. If TA and TB are the time period of star A and star B, respectively, then: