Gravitation
- A black hole is an object whose gravitational field is so strong that even light cannot escape from it. To what approximate radius would earth (mass = 5.98 × 1024 kg) have to be compressed to be a black hole?
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From question, Escape velocity = √2GM / R = c = speed of light
⇒ R = 2GM c2 = 2 × 6.6 × 10-11 × 5.98 × 1024 = 10-2 m (3 × 108)2 Correct Option: C
From question, Escape velocity = √2GM / R = c = speed of light
⇒ R = 2GM c2 = 2 × 6.6 × 10-11 × 5.98 × 1024 = 10-2 m (3 × 108)2
- The height at which the weight of a body becomes 1/16th, its weight on the surface of earth (radius R), is :
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Let at h height, the weight of a body becomes 1 th of its weight on the surface. 16
Wh = 16 Ws....(i)
⇒16 Ws = Ws....(ii)g' = G M (Re + h)2 Similarly , g = G M Re2 g' = Re2 ⇒ g' = g 1 + h -2 g (Re + h)2 R
⇒ Wh = 16 Wsg' = g 16 g' = 16g 1 + h 2 R 1 = 1 + h -2 ⇒ 4 = 1 + h 16 R R
h = 3R
Correct Option: C
Let at h height, the weight of a body becomes 1 th of its weight on the surface. 16
Wh = 16 Ws....(i)
⇒16 Ws = Ws....(ii)g' = G M (Re + h)2 Similarly , g = G M Re2 g' = Re2 ⇒ g' = g 1 + h -2 g (Re + h)2 R
⇒ Wh = 16 Wsg' = g 16 g' = 16g 1 + h 2 R 1 = 1 + h -2 ⇒ 4 = 1 + h 16 R R
h = 3R
- A satellite A of mass m is at a distance of r from the surface of the earth. Another satellite B of mass 2m is at a distance of 2r from the earth’s centre. Their time periods are in the ratio of
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Time period does not depend on the mass.
Also, T2 ∝ r3 .Correct Option: D
Time period does not depend on the mass.
Also, T2 ∝ r3 .