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NEET PHYSICSMedium

The ratio of escape velocity at the Earth (vev_e) to the escape velocity at a planet (vpv_p) whose radius and mean density are twice that of the Earth is:

A

1 : 2\sqrt{2}

B

1 : 4

C

1 : \sqrt{2}

D

1 : 2

Step-by-Step Solution

  1. Escape Velocity Formula: The escape velocity vev_e from a spherical body of mass MM and radius RR is given by ve=2GMRv_e = \sqrt{\frac{2GM}{R}} .
  2. In Terms of Density: To relate velocity to density (ρ\rho), express mass as M=Volume×Density=43πR3ρM = \text{Volume} \times \text{Density} = \frac{4}{3}\pi R^3 \rho. Substituting this into the escape velocity formula: v=2GR(43πR3ρ)=8πGρR23v = \sqrt{\frac{2G}{R} \left( \frac{4}{3}\pi R^3 \rho \right)} = \sqrt{\frac{8\pi G \rho R^2}{3}} From this, we see that vRρv \propto R\sqrt{\rho}.
  3. Ratio Calculation: Let Earth's radius be RR and density be ρ\rho. Then the planet has radius R=2RR' = 2R and density ρ=2ρ\rho' = 2\rho. vevp=RρRρ=Rρ(2R)2ρ\frac{v_e}{v_p} = \frac{R\sqrt{\rho}}{R'\sqrt{\rho'}} = \frac{R\sqrt{\rho}}{(2R)\sqrt{2\rho}} vevp=122\frac{v_e}{v_p} = \frac{1}{2\sqrt{2}} The ratio is 1:221 : 2\sqrt{2}.
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