Two bodies (binary system) of mass M and m(M>m) revolve in circular orbits of radii R and r, respectively about their centre of mass. Their angular speeds are ω1 and ω2. Then :
A
ω1R=ω2r
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B
ω1r=ω2R
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C
ω1=ω2
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D
ω21R=ω22r
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Solution
The correct option is Cω1=ω2 They revolve around their center of mass of system, So mr = MR →mR=Mr
The gravitational force between them acts as centripetal force.
Thus,
GMm(R+r)2=m(ω1)2r=M(ω2)2R
Solving this, we get ω1=(GMr(R+r)2)0.5=(GmR(R+r)2)0.5=ω2