Satellites A and B are orbiting around the earth in orbits of ratio R and 4R respectively. The ratio of their areal velocities is-
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Using Kepler's second law we have:
Arealvelocity=
time
Areaswept
=
dt
2
1
r(rdθ)
=
2
1
r
2
ω=
2
1
rv=constant
Thus we get,
2
1
r
GM
r (from
r
mv
2
=
r
2
GMm
)
Thus we get
Areal velocity ∝
r
Thus for the planets with radius in ratio of 1:4 we get radii in the ratio of 1:2
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