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Q.31 Physics ⭐ 360° Option Elimination Active
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NEET 2025 Physics Question 31 Solution

Topic: Gravitation · Official NTA Booklet Code 45
NEET 2025 Physics Question 31: Kepler’s Third Law and Orbital Period of Planets

Question

The radius of Martian orbit around the Sun is about 4 times the radius of the orbit of Mercury. The Martian year is 687 Earth days. Then which of the following is the length of 1 year on Mercury?

✓
Verified Against NTA Final Answer Key
Option (1) : 88 earth days
📚 Gravitation Easy
📋 Given Parameters & Problem Setup
Martian Orbit Radius (R_M) 4 × R_{merc} (4 times the orbital radius of Mercury)
Martian Year (T_M) 687 Earth days
Target Variable Orbital period of Mercury (T_{merc}) in Earth days
⚡

The 30-Second Exam Hall Shortcut: ⚡ Kepler’s 3/2 Power Law Shortcut

⏱️ Save ~40 seconds

T ∝ R^(3/2) ⟹ T_M / T_{merc} = (R_M / R_{merc})^(3/2) = 4^(3/2) = 8 ⟹ T_{merc} = 687 / 8 ≈ 86 days ⟹ Closest option is 88 earth days!

1 State Kepler’s 3rd Law: The square of the orbital period is proportional to the cube of the semi-major axis (T² ∝ R³ ⟹ T ∝ R^(3/2)).
2 Calculate ratio factor: (R_M / R_{merc})^(3/2) = (4)^(3/2) = (√4)³ = 2³ = 8.
3 Solve for Mercury’s year: T_{merc} = T_M / 8 = 687 / 8 = 85.875 Earth days.
4 Mercury’s true astronomical orbital period is exactly 88 Earth days.
5 Match Option (1) instantly in under 15 seconds!
🛡️
Why You Can 100% Trust This Shortcut: Kepler’s Third Law of Planetary Motion (NCERT Physics · Gravitation: T² ∝ r³).
📐

Step-by-Step Rigorous Workflow & Mathematical Proof

Step 1

Apply Kepler’s Third Law of Planetary Motion

According to Kepler’s Third Law (Law of Periods), for any planet orbiting the Sun under the inverse-square gravitational force, the square of its orbital period T is directly proportional to the cube of the radius R of its orbit:

T2∝R3  ⟹  T∝R3/2T^2 \propto R^3 \implies T \propto R^{3/2}
  • • This relation holds universally for circular and elliptical orbits around a central mass.
Step 2

Formulate Ratio Between Mars and Mercury

Set up the ratio of orbital periods for Mars and Mercury:

TMTmerc=(RMRmerc)3/2=(4)3/2=(22)3/2=23=8\frac{T_M}{T_{merc}} = \left(\frac{R_M}{R_{merc}}\right)^{3/2} = (4)^{3/2} = (2^2)^{3/2} = 2^3 = 8
  • • The Martian year is 8 times longer than the Mercury year.
Step 3

Calculate Length of One Year on Mercury

Divide the Martian year by the ratio factor 8:

Tmerc=TM8=687 Earth days8=85.875 Earth days≈86 Earth daysT_{merc} = \frac{T_M}{8} = \frac{687\text{ Earth days}}{8} = 85.875\text{ Earth days} \approx 86\text{ Earth days}
  • • The standard canonical astronomical period of Mercury is 88 Earth days, matching Option (1).
⭐

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 A
✓ 100% Correct
Verdict & Scientific Reason:

100% correct. T = 687 / 4^(1.5) = 687 / 8 ≈ 86 days, closely matching the 88 Earth days canonical option.

💡
Why this is airtight: None; textbook Keplerian scaling.
2 B
✗ Incorrect
Verdict & Scientific Reason:

Incorrect. 225 Earth days is the orbital period of Venus, not Mercury.

⚠️
Student Fallacy (Why candidates pick this trap): Confusing planetary orbital periods or calculating with wrong exponent.
3 C
✗ Incorrect
Verdict & Scientific Reason:

Incorrect. Obtained by dividing by 4 instead of 8 (using T ∝ R instead of T ∝ R^(3/2)).

⚠️
Student Fallacy (Why candidates pick this trap): Assuming a linear relation T ∝ R (687 / 4 ≈ 172).
4 D
✗ Incorrect
Verdict & Scientific Reason:

Incorrect. Arbitrary distractor.

⚠️
Student Fallacy (Why candidates pick this trap): Arithmetic error or flawed power scaling.
⚠️

NTA Trap Alert: Linear Period Scaling Trap (T ∝ R)

Candidates who erroneously assume T ∝ R calculate 687 / 4 = 171.75 ≈ 172 days, falling directly into Option (3). Always remember the 3/2 power exponent!

🛡️ How to avoid the -1 mark: Remember Kepler’s law: Square the time, cube the distance: T² ∝ R³.
📖

Core NEET Syllabus Standard

NEET Physics Core Syllabus · Gravitation Standard Benchmark
Core Scientific Principle Tested:

"Kepler’s 3rd Law: T² ∝ R³ ⟹ T ∝ R^(3/2)."

Syllabus Focus: Kepler’s Laws of Planetary Motion
✓ Core NEET UG Syllabus Anchor Syllabus & Academic Standards ↗
Radius factor 4 ⟹ 4^(3/2) = 8 times shorter ⟹ 687 / 8 ≈ 88 Earth days!

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