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A spherically symmetric gravitational system of particles has a mass density ρ={ρ0 for r≤R0 for r>Rwhere ρ0 is a constant. A test mass can undergo circular motion under the influence of the gravitational field of particles. Its speed V as a function of distance r(0<r<∞) from the centre of the system is represented by

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A spherically symmetric gravitational system of particles has a mass density ρ={ρ0 for rR0 for r>R

where ρ0 is a constant. A test mass can undergo circular motion under the influence of the gravitational field of particles. Its speed V as a function of distance r(0<r<) from the centre of the system is represented by



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