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Question: A satellite A of mass m is at a distance of r from the centre of the earth. Another satellite B of m...

A satellite A of mass m is at a distance of r from the centre of the earth. Another satellite B of mass 2m is at distance of 2r from the earth’s centre. Their time periods are in the ratio of

A

1 : 2

B

1 : 16

C

1 : 32

D

1:221 : 2 \sqrt { 2 }

Answer

1:221 : 2 \sqrt { 2 }

Explanation

Solution

Time period does not depend upon the mass of satellite, it only depends upon the orbital radius.

According to Kepler's law =(r2r)3/2= \left( \frac { r } { 2 r } \right) ^ { 3 / 2 } =122= \frac { 1 } { 2 \sqrt { 2 } }