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Escape velocity ratio of stars after mass transfer

Two spherical stars AA and BB have densities ρA\rho_A and ρB\rho_B, respectively. AA and BB have the same radius, and their masses MAM_A and MBM_B are related by MB=2MAM_B = 2M_A. Due to an interaction process, star AA loses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density remains ρA\rho_A. The entire mass lost by AA is deposited as a thick spherical shell on BB with the density of the shell being ρA\rho_A. If vAv_A and vBv_B are the escape velocities from AA and BB after the interaction process, the ratio vBvA=10n151/3\frac{v_B}{v_A} = \sqrt{\frac{10n}{15^{1/3}}}. The value of nn is ____.

Official Numerical Answer2.3

Topics & Concepts

Step-by-Step Solution

To find the value of nn, we analyze the parameters of stars AA and BB before and after the interaction process.

1. Initial Parameters of Stars AA and BB

Let RR be the initial radius of both spherical stars AA and BB.

  • The initial mass of star AA is MAM_A, given by: MA=43πR3ρAM_A = \frac{4}{3} \pi R^3 \rho_A
  • The initial mass of star BB is MB=2MAM_B = 2M_A.

2. Parameters of Star AA After Mass Transfer

After the interaction:

  • The radius of star AA becomes RA=R2R_A' = \frac{R}{2}.
  • The density remains ρA\rho_A.

The new mass of star AA, MAM_A', is: MA=43π(R2)3ρA=18(43πR3ρA)=MA8M_A' = \frac{4}{3} \pi \left(\frac{R}{2}\right)^3 \rho_A = \frac{1}{8} \left(\frac{4}{3} \pi R^3 \rho_A\right) = \frac{M_A}{8}

The mass lost by star AA is: ΔM=MAMA=MAMA8=78MA\Delta M = M_A - M_A' = M_A - \frac{M_A}{8} = \frac{7}{8} M_A


3. Parameters of Star BB After Mass Transfer

The mass lost by AA, ΔM\Delta M, is deposited as a thick spherical shell on BB with density ρA\rho_A.

  • Inner radius of the shell = RR
  • Let RBR_B' be the outer radius of star BB with the shell.

The volume of the shell is: Vshell=43π((RB)3R3)V_{\text{shell}} = \frac{4}{3} \pi \left((R_B')^3 - R^3\right)

Since the mass of the shell is ΔM\Delta M: 43π((RB)3R3)ρA=78MA=78(43πR3ρA)\frac{4}{3} \pi \left((R_B')^3 - R^3\right) \rho_A = \frac{7}{8} M_A = \frac{7}{8} \left(\frac{4}{3} \pi R^3 \rho_A\right)

Canceling common terms: (RB)3R3=78R3(R_B')^3 - R^3 = \frac{7}{8} R^3 (RB)3=158R3    RB=151/32R(R_B')^3 = \frac{15}{8} R^3 \implies R_B' = \frac{15^{1/3}}{2} R

The total mass of star BB after the interaction is: MB=MB+ΔM=2MA+78MA=238MAM_B' = M_B + \Delta M = 2M_A + \frac{7}{8} M_A = \frac{23}{8} M_A


4. Ratio of Escape Velocities

The escape velocity from a spherical body of mass MM and radius rr is given by: v=2GMrv = \sqrt{\frac{2GM}{r}}

  • Escape velocity from AA (vAv_A): vA=2GMARA=2G(MA8)R2=GMA2Rv_A = \sqrt{\frac{2 G M_A'}{R_A'}} = \sqrt{\frac{2 G \left(\frac{M_A}{8}\right)}{\frac{R}{2}}} = \sqrt{\frac{G M_A}{2 R}}

  • Escape velocity from BB (vBv_B): vB=2GMBRB=2G(238MA)151/32R=23GMA2151/3Rv_B = \sqrt{\frac{2 G M_B'}{R_B'}} = \sqrt{\frac{2 G \left(\frac{23}{8} M_A\right)}{\frac{15^{1/3}}{2} R}} = \sqrt{\frac{23 G M_A}{2 \cdot 15^{1/3} R}}

  • Ratio vBvA\frac{v_B}{v_A}: vBvA=23GMA2151/3RGMA2R=23151/3\frac{v_B}{v_A} = \frac{\sqrt{\frac{23 G M_A}{2 \cdot 15^{1/3} R}}}{\sqrt{\frac{G M_A}{2 R}}} = \sqrt{\frac{23}{15^{1/3}}}


5. Determination of nn

Comparing the derived ratio with the given expression: 23151/3=10n151/3\sqrt{\frac{23}{15^{1/3}}} = \sqrt{\frac{10n}{15^{1/3}}}

Equating the numerators inside the square root: 10n=23    n=2.310n = 23 \implies n = 2.3