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PhysicsGravitationEnergy & PotentialMedium2 minPYQ_2022
PhysicsMediumnumerical

Two spherical starsAandBhave densitiesρAandρB, respectively.AandBhave the same radius, and their massesMAandMBare related byMB=2MA. Due to an interaction process, starAloses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density remainsρA. The entire mass lost byAis deposited as a thick spherical shell onBwith the density of the shell beingρA. IfvAandvBare the escape velocities fromAandBafter the interaction process, the ratiovBvA=10n1513. The value ofnis

Answer:
2.30
Solution:

Given here: RA=RB=R and MB=2MA.

Now, after interaction process, radius of remaining star A is RA'=R2 and its mass is MA'=ρA43πRA23=MA8

Applying conservation of energy,

 -GMA'mRA'+12mvA2=0

Escape velocity of star A is vA=2GMA8×R2=v02

Now, for B, mass collected over B is MB'=MA-MA8=78MA.

Let the radius of star B after interaction becomes r.

Applying mass conservation, 

43πr3-R3ρA=43πR3×78ρA

r=15813R

Escape velocity of star B is 

 vB=2G×2MA+78MA151/3R2

=2GMAR216+781513

=v0×23×28×1513=v02×231513

Now, the ratio vBvA=231513=2.30×101513

 n=2.30

Stream:JEE_ADVSubject:PhysicsTopic:GravitationSubtopic:Energy & Potential
2mℹ️ Source: PYQ_2022

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