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Consider a spherical gaseous cloud of mass density ρ(r) in a free space where r is the radial distance from its centre. The gaseous cloud is made of particles of equal mass m moving in circular orbits about their common centre with the same kinetic energy K. The force acting on the particles is their mutual gravitational force. If ρ(r) is constant with time. The particle number density n(r) = ρ(r)/m is:

(g = universal gravitational constant)

a) 3K/πr2m2G b) K/2πr2m2G c) K/πr2m2G d) K/6πr2m2G Answer: (b) GMm/r = mv2/r = 2/r x ½ x mv2 = 2k/r M = 2kr/Gm 4πr2 dr ρ = 2k dr/Gm Or ρ... View Article