if ρ is the mean density of the earth and R is the radius then the time period of the satellite revolving close to the surface is
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formula for time period=
2π(√(R+h)³/GM)
where,
R=radius of earth
h=height of settelite
G=universal gravitational constant
M=mass of earth
now;
if
h is very very less, for a satellite revolving close to earth,(negligible)
t=2π(√(R)³/GM)
we know;
density=mass/volume
ρ=M/4πR³ volume=4πR³
M=ρ4πR³
substituting these values in the formula of time period, we get;
t=2π(√(R)³/Gρ4πR³)
t=2π(√1/Gρ4π)
t=√π/Gρ
answer:t=√π/Gρ
diyamehta2611:
but there is no option such like that.
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