Question Details

Two spherical stars A and B have densities ρA and ρB, respectively. A and B have the same radius, and their masses MA and MB are related by MB = 2MA. Due to an interaction process, star A loses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density remains ρA. The entire mass lost by A is deposited as a thick spherical shell on B with the density of the shell being ρA. If vA and vB are the escape velocities from A and B after the interaction process, the ratio
vBvA=10n1513
The value of n is ______.

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Correct Answer :

2.30

Solution :

The correct answer is 2.30.

Step 1: Initial Parameters

Let the initial radius of stars A and B be R.
Initial mass of star A is MA=43πR3ρA
Initial mass of star B is MB=2MA

Step 2: Properties of Star A After Interaction

The radius of star A becomes RA=R2 while keeping density ρA constant.
New mass of star A:

MA=43πR23ρA=MA8

Mass lost by star A:

ΔM=MAMA8=78MA

Escape velocity from star A after interaction:

vA=2GMARA=2GMA8R2=GMA2R

Step 3: Properties of Star B After Interaction

New mass of star B:

MB=MB+ΔM=2MA+78MA=238MA

The added shell has density ρA, so the outer radius RB of B is given by:

43πRB343πR3=ΔMρA=7843πR3

RB3=R3+78R3=158R3RB=15132R

Escape velocity from star B after interaction:

vB=2GMBRB=2G23MA815132R=23GMA2·1513R

Step 4: Finding the Ratio and Solving for n

vBvA=23GMA2·1513RGMA2R=231513

Equating this to the given relation:

231513=10n1513

10n=23n=2.30

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