The ratio of distance of two satellites from the centre of earth is 1 : 4. The ratio of their time periods of rotation will be :
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Answered by
14
Answer:
Ratio b/w distance from to satellite= 1: 4
R1 = 1 x and R2 = 4x
According to Kepler's Third law the formula for time period of a satellite :
= (T1/ T2 )^2 = ( R1 /R2 ) ^3
= ( T1/ T2 )^2 = ( 1x / 4x ) ^3
= (T1/T2 )^2 = 1/64
= T1 / T2 = root ( 1/ 64 )
= T1/ T2 = 1/8
So , T1 = 1 hour
and
T2 = 8 hours
Hope it helps you!
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Answered by
2
Time period is not dependent on mass of satellite.
Time period(T) = 2π√r³/√GM ( M is mass of earth)
T² is directly proportional to r³
Therefore,
Ratio = r³/(2r)³
= r³/8r³
= 1:8
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