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Q.34 Physics ⭐ 360° Option Elimination Active
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NEET 2021 Physics Question 34 Solution

Topic: Gravitation · Official NTA Booklet Code M1
NEET 2021 Physics Question 34: Escape Velocity in Terms of Radius and Constant Planetary Mass Density

Question

The escape velocity from the Earth's surface is v. The escape velocity from the surface of another planet having a radius, four times that of Earth and same mass density is:

✓
Verified Against NTA Final Answer Key
Option (4) : 4v
📚 Gravitation Easy
📋 Given Parameters & Problem Setup
Escape Velocity on Earth v
New Planet Radius (R') 4 R_E
New Planet Density (ρ') Equal to Earth (same mass density ρ)
⚡

The 30-Second Exam Hall Shortcut: ⚡ Constant Density Escape Velocity Shortcut: v_e ∝ R

⏱️ Save ~20 seconds

ve=2GMR=2G(43πR3ρ)R=R83πGρ  ⟹  ve∝Rv_e = \sqrt{\frac{2GM}{R}} = \sqrt{\frac{2G(\frac{4}{3}\pi R^3 \rho)}{R}} = R \sqrt{\frac{8}{3}\pi G \rho} \implies v_e \propto R! Since the planet's radius is 4 times that of Earth at identical density, the escape velocity is directly 4v4v! Instant 5-second answer matching Option (4)!

1 Express mass in terms of density: M=43πR3ρM = \frac{4}{3}\pi R^3 \rho.
2 Substitute into escape velocity formula: ve=2GMR=2GR(43πR3ρ)=R83πGρv_e = \sqrt{\frac{2G M}{R}} = \sqrt{\frac{2G}{R} \left(\frac{4}{3}\pi R^3 \rho\right)} = R \sqrt{\frac{8}{3}\pi G \rho}.
3 For equal mass density (ρ=constant\rho = \text{constant}), ve∝Rv_e \propto R.
4 Since R′=4RR' = 4 R, we have v′=4vv' = 4 v.
5 Match Option (4).
🛡️
Why You Can 100% Trust This Shortcut: Canonical Newton's law of gravitation and spherical planetary mass-density integration.
📐

Step-by-Step Rigorous Workflow & Mathematical Proof

Step 1

Standard Formula for Escape Velocity

The minimum velocity required for a particle to escape gravitational attraction from the surface of a spherical planet of mass MM and radius RR is:

ve=2GMRv_e = \sqrt{\frac{2GM}{R}}
Step 2

Expressing Escape Velocity in Terms of Density

Assuming uniform mass density ρ\rho, the planetary mass is M=43πR3ρM = \frac{4}{3}\pi R^3 \rho. Substituting into the escape velocity formula gives:

ve=2G(43πR3ρ)R=83πGρR2=R8πGρ3v_e = \sqrt{\frac{2G \left(\frac{4}{3}\pi R^3 \rho\right)}{R}} = \sqrt{\frac{8}{3}\pi G \rho R^2} = R \sqrt{\frac{8\pi G \rho}{3}}
Step 3

Comparing the New Planet with Earth

For two planets of identical density ρ\rho, escape velocity is directly proportional to planetary radius:

v′v=R′R=4RR=4  ⟹  v′=4v\frac{v'}{v} = \frac{R'}{R} = \frac{4R}{R} = 4 \implies v' = 4v
⭐

360° Option Elimination Engine Key Feature

Diagnose every choice: Know exactly why the right option works and why distractors fail.

4-Option Deep Scan
1 1
✗ Incorrect
Verdict & Scientific Reason:

Assumes escape velocity is independent of planetary radius.

⚠️
Student Fallacy (Why candidates pick this trap): Believing escape speed is a universal constant.
2 2
✗ Incorrect
Verdict & Scientific Reason:

Result of applying ve∝Rv_e \propto \sqrt{R}, which only applies if planet MASS is held constant (M=constM = \text{const}), not density.

⚠️
Student Fallacy (Why candidates pick this trap): Using ve=2GM/Rv_e = \sqrt{2GM/R} with constant MM instead of constant ρ\rho.
3 3
✗ Incorrect
Verdict & Scientific Reason:

Unphysical integer guess.

⚠️
Student Fallacy (Why candidates pick this trap): Random estimation.
4 4
✓ 100% Correct
Verdict & Scientific Reason:

Exact escape velocity for a planet with 4×4\times radius and identical density (ve∝Rv_e \propto R).

💡
Why this is airtight: None; rigorous gravitational density scaling.
⚠️

NTA Trap Alert: Constant Mass vs. Constant Density Proportionality Trap

If planetary MASS is constant: ve∝1Rv_e \propto \frac{1}{\sqrt{R}}. If planetary DENSITY is constant: M∝R3M \propto R^3, making ve∝Rv_e \propto R. Candidates who mistakenly use constant mass obtain v/2v/2 or 2v2v (Option 2).

🛡️ How to avoid the -1 mark: Identify the invariant: "same mass density"   ⟹  ve∝R\implies v_e \propto R. Since RR is 4×4\times, vv is 4×4\times.
📖

Core NEET Syllabus Standard

NCERT Physics · Gravitation Standard Benchmark
Core Scientific Principle Tested:

"Escape velocity from a celestial body of uniform density ρ\rho and radius RR is ve=R8πGρ3v_e = R\sqrt{\frac{8\pi G\rho}{3}}, which scales linearly with radius."

Syllabus Focus: Escape Speed
✓ Core NEET UG Syllabus Anchor Syllabus & Academic Standards ↗

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