The magnitude of the gravitational force experienced by a small spaceship of mass M inside an
inter-galactic dust cloud (assumed to be spherically symmetric but not necessarily uniform) when
it at a distance of r from the center of the cloud is found to be
F(r) = αr +
β
r
.
The density of the dust cloud is (G is Newton’s gravitational constant)
A. 3α
4πGM
1 −
β
3αr
2
B. 3α
4πGM
1 +
β
3αr
2
C. 3α
4πGM
1 +
β
αr
2
D. 3α
4πGM
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