Suppose the gravitational force varies inversely as the nth powe

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21.

Suppose the gravitational force varies inversely as the nth power of distance. Then the time period planet in circular orbit of radius R around the sun will be proportional to

  • straight R to the power of open parentheses fraction numerator straight n plus 1 over denominator 2 end fraction close parentheses end exponent
  • straight R to the power of open parentheses fraction numerator straight n minus 1 over denominator 2 end fraction close parentheses end exponent
  • Rn

  • Rn


A.

straight R to the power of open parentheses fraction numerator straight n plus 1 over denominator 2 end fraction close parentheses end exponent

The necessary centripetal force required for a planet to move round the sun = gravitational force exerted on it

straight i. straight e space mv squared over straight R space equals space fraction numerator GM subscript straight e straight m over denominator straight R end fraction
straight v space equals space open parentheses GM over straight R to the power of straight n minus 1 end exponent close parentheses to the power of 1 divided by 2 end exponent
Now comma space straight T space equals space fraction numerator 2 πR over denominator straight v end fraction space equals space 2 πRx space open parentheses straight R to the power of straight n minus 1 end exponent over GM subscript straight e close parentheses to the power of 1 divided by 2 end exponent
space equals space 2 straight pi space open parentheses fraction numerator straight R squared space straight x space straight R to the power of straight n minus 1 end exponent over denominator GM subscript straight e end fraction close parentheses to the power of 1 divided by 2 end exponent
space equals space 2 straight pi space open parentheses fraction numerator straight R to the power of left parenthesis straight n plus 1 right parenthesis divided by 2 end exponent over denominator left parenthesis GM subscript straight e right parenthesis to the power of 1 divided by 2 end exponent end fraction close parentheses
straight T space proportional to space straight R to the power of left parenthesis straight n plus 1 right parenthesis divided by 2 end exponent

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22.

A comet orbits around the Sun in an elliptical orbit. Which of the following quantities remains constant during the course of its motion ?

  • Linear velocity

  • Angular velocity

  • Angular momentum

  • Kinetic energy


23.

Consider a satellite moving in a circular orbit around Earth. If K and V denote its kinetic energy and potential energy respectively, then (Choose the convention, where V = 0 as r → ∞)

  • K = V

  • K = 2V

  • V = − 2K

  • K = − 2V


24.

Assuming the mass of Earth to be ten times the mass of Mars, its radius to be twice the radius of Mars and the acceleration due to gravity on the surface of Earth is 10 m/s2. Then the acceleration due to gravity on the surface of Mars is given by

  • 0.2 m/s2

  • 0.4 m/s2

  • 2 m/s2

  • 4 m/s2


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25.

The semi-major axis of the orbit of Saturn is approximately nine times that of Earth. The time period of revolution of Saturn is approximately equal to

  • 81 years

  • 27 years

  • 729 years

  • 813 years


26.

A body hanging from a massless spring stretches it by 3 cm on Earth's surface. At a place 800 km above the Earth's surface, the same body will stretch the spring by (Radius of Earth = 6400 km)

  • 3427 cm

  • 6427 cm

  • 2764 cm

  • 2734 cm


27.

The acceleration due to gravity on the surface of a planet is one-fourth of the value on Earth. When a brass ball is brought to this planet, its

  • mass is halved

  • weight is halved

  • mass becomes one-fourth

  • weight becomes one-fourth


28.

Polar satellites

  • are high altitude satellite

  • are widely used for telecommunication

  • are used for environmental studies

  • go around the Earth in a East-West direction


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29.

Angular momentum of the Earth revolving around the Sun in a circular orbit of radius R is proportional to

  • R

  • R

  • R2

  • R1/3


30.

A body of mass m is released from a height equal to the radius R of the Earth. The velocity with which it will strike the Earth's surface is

  • 2gR

  • gR

  • 2 mgR

  • mgR


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