1. Law of orbits: planets orbit the Sun in ellipses with the Sun at one focus. 2. Law of areas: the line from Sun to planet sweeps equal areas in equal times (consequence of angular momentum conservation). 3. Law of periods: T² ∝ r³, where r is the semi-major axis.
-- NCERT Class 11 Physics, Ch. 7, p. 129Kepler's Laws
Kepler's Laws, explained for NEET
The trap: When a planet's orbital radius doubles, most students instinctively double the period. That loses you marks. The period does not scale linearly with radius — it scales as the 3/2 power.
Kepler's three laws (NCERT Class 11 Physics Chapter 7, page 129):
- Law of orbits. Every planet moves in an ellipse with the Sun at one focus — not at the centre.
- Law of areas. The line joining the planet and the Sun sweeps equal areas in equal time intervals. This means the planet moves faster near perihelion (closest approach) and slower near aphelion (farthest point). No external torque about the Sun → angular momentum is conserved.
- Law of periods. T² ∝ a³, where T is the orbital period and a is the semi-major axis. For two planets orbiting the same star: (T₁/T₂)² = (a₁/a₂)³.
Why the third law trips you in NEET: The relationship T ∝ a^(3/2) is non-linear. Doubling the semi-major axis multiplies the period by 2^(3/2) = 2√2 ≈ 2.83 — not 2. Quadrupling a gives T → 4^(3/2) = 8 times the original period. NEET questions routinely offer the linear-scaling answer as a distractor.
Deriving T² ∝ a³ for circular orbits. For a circular orbit of radius r, equating gravitational force to centripetal force:
GMm/r² = mv²/r → v² = GM/r
Period T = 2πr/v, so T² = 4π²r³/(GM). This confirms T² ∝ r³ with the proportionality constant depending only on the central mass M, not on the orbiting body's mass.
Watch out: Kepler's third law compares orbits around the same central body. You cannot use T₁²/T₂² = a₁³/a₂³ to compare a planet orbiting the Sun with a satellite orbiting Earth — the central masses differ.
Can you answer these Kepler's Laws MCQs?
Select an option to see the explanation. Wrong answers show why your choice was tempting — and name the exact trap it exploits.
According to Kepler's first law, every planet moves in an orbit that is:
Show answer and why every option is right or wrong
Answer: D. Kepler's first law states that planetary orbits are ellipses with the Sun at one focus (NCERT Class 11 Physics Chapter 7, page 129).
Why A is wrong: A is wrong because Kepler corrected the circular-orbit assumption; orbits are elliptical, and the Sun is at a focus, not the geometric centre.
Why B is wrong: B is wrong because while the shape is an ellipse, the Sun occupies one focus — not the centre. The centre of an ellipse is equidistant from both foci.
Why C is wrong: C is wrong because a parabola describes an unbound trajectory (escape path), not a bound planetary orbit.
Kepler's second law (law of areas) is a direct consequence of conservation of:
Show answer and why every option is right or wrong
Answer: D. The gravitational force is central (directed along the radius vector), so torque about the Sun is zero and angular momentum is conserved. Equal areas in equal times follows from L = constant (NCERT Class 11 Physics Chapter 7, page 129).
Why A is wrong: A is wrong because the gravitational force continuously changes the planet's direction, so linear momentum is not conserved. It is angular momentum (about the Sun) that is conserved due to zero torque.
Why B is wrong: B is wrong because while total energy is conserved in the orbit, the equal-area law follows specifically from angular momentum conservation (zero torque), not from the energy equation.
Why C is wrong: C is wrong because mass conservation is trivially true for the planet but has no connection to the areal velocity being constant.
A planet at perihelion is at distance r₁ from the Sun and has speed v₁. At aphelion the distance is r₂. What is the speed at aphelion?
Show answer and why every option is right or wrong
Answer: B. By conservation of angular momentum (Kepler's second law), m v₁ r₁ = m v₂ r₂, giving v₂ = v₁ r₁ / r₂ (NCERT Class 11 Physics Chapter 7, page 129).
Why A is wrong: A is wrong because it inverts the ratio. Since r₂ > r₁, this would make the aphelion speed greater than perihelion speed, contradicting Kepler's second law (planet moves slower when farther).
Why C is wrong: C is wrong because it uses an inverse-square ratio of distances. Angular momentum conservation gives a linear ratio (v ∝ 1/r for the transverse component), not an inverse-square one.
Why D is wrong: D is wrong because it applies the square of the distance ratio in the wrong direction, yielding a speed much larger at aphelion — the opposite of what Kepler's law requires.
The orbital period of planet A around a star is T. Planet B orbits the same star with a semi-major axis twice that of planet A. The orbital period of B is:
Show answer and why every option is right or wrong
Answer: C. By Kepler's third law, T² ∝ a³. If a₂ = 2a₁, then T₂² = 2³ T₁² = 8T₁², so T₂ = √8 T = 2√2 T (NCERT Class 11 Physics Chapter 7, page 129). (Trap: treating T as proportional to a gives the wrong answer 2T.)
Why A is wrong: A is wrong because it assumes T ∝ a (linear scaling). Kepler's third law gives T ∝ a^(3/2), so doubling a multiplies T by 2^(3/2) = 2√2, not 2. This is a common NEET distractor exploiting the linear-scaling confusion.
Why B is wrong: B is wrong because it assumes T ∝ a² (square scaling). Kepler's third law gives T² ∝ a³, i.e., T ∝ a^(3/2). Doubling a gives T₂ = 2^(3/2) T = 2√2 T ≈ 2.83T, not 4T.
Why D is wrong: D is wrong because it uses T ∝ a³. While T² ∝ a³ is correct, taking the square root gives T ∝ a^(3/2), so T₂ = 2^(3/2) T = 2√2 T, not 2³ T = 8T.
If the semi-major axis of a planet's orbit is increased by a factor of 4, the orbital period increases by a factor of:
Show answer and why every option is right or wrong
Answer: A. T ∝ a^(3/2). Factor = 4^(3/2) = (√4)³ = 2³ = 8 (NCERT Class 11 Physics Chapter 7, page 129). (Trap: linear scaling gives 4; square scaling gives 16.)
Why B is wrong: B is wrong. There is no standard power law that yields a factor of 6 from a 4× change in a. Kepler's law gives T ∝ a^(3/2), so the factor is 4^(3/2) = 8.
Why C is wrong: C is wrong because it assumes T scales linearly with a. Kepler's third law gives T ∝ a^(3/2), so quadrupling a multiplies T by 4^(3/2) = 8, not 4.
Why D is wrong: D is wrong because it assumes T ∝ a² (i.e., T factor = 4² = 16). The correct relation is T ∝ a^(3/2), giving 4^(3/2) = 8.
A satellite is in a circular orbit around Earth. If its orbital radius is increased 25-fold, by what factor does its orbital period change?
Show answer and why every option is right or wrong
Answer: C. First derive how speed depends on radius: equating gravitational force to centripetal force, GMm/r² = mv²/r, gives v² = GM/r, so v ∝ 1/√r. Increasing r by 25× therefore decreases v by a factor of √25 = 5, i.e., v_new = v_old/5 — this is a separate result, not given in the stem. Second, feed that result into T = 2πr/v: T_new/T_old = (r_new/r_old) × (v_old/v_new) = 25 × 5 = 125. Neither step alone gives the answer; the velocity-scaling result from the force balance must be produced first and then substituted into the period relation (NCERT Class 11 Physics Chapter 7, page 129).
Why A is wrong: A is wrong because it applies only the √25 = 5 velocity-scaling factor on its own, forgetting that T = 2πr/v also carries an explicit factor of r itself; both the radius change and the resulting velocity change must enter T's scaling.
Why B is wrong: B is wrong because it applies only the radius factor (r × 25) to T, treating v as if it stayed constant — but the force-balance relation v ∝ 1/√r shows v also changes with r, and that change must be folded into T = 2πr/v.
Why D is wrong: D is wrong because it multiplies the radius factor by itself (25 × 25) instead of by the velocity factor (25 × 5); since v ∝ 1/√r gives v_new = v_old/5 (not v_old/25), the correct combination is 25 × 5 = 125, not 625.
A planet sweeps area A in time Δt when it is near perihelion. When the same planet is near aphelion, the area swept in the same time Δt is:
Show answer and why every option is right or wrong
Answer: C. Kepler's second law states equal areas are swept in equal time intervals, regardless of the planet's position in its orbit (NCERT Class 11 Physics Chapter 7, page 129). The areal velocity dA/dt is constant.
Why A is wrong: A is wrong because although the orbital radius is larger at aphelion, the planet's speed is correspondingly slower. Kepler's second law guarantees the area swept per unit time is the same everywhere in the orbit.
Why B is wrong: B is wrong for the same reason — the slower speed at aphelion exactly compensates for the larger radius, keeping dA/dt constant.
Why D is wrong: D is wrong because Kepler's second law holds for all elliptical orbits regardless of eccentricity. No additional information is needed.
Planet X orbits a star with period 27 years and semi-major axis a_X. Planet Y orbits the same star with semi-major axis a_Y = a_X / 3. The orbital period of Y is:
Show answer and why every option is right or wrong
Answer: B. T_Y/T_X = (a_Y/a_X)^(3/2) = (1/3)^(3/2) = 1/(3√3). So T_Y = 27/(3√3) = 27/(3 × 1.732) = 9/1.732 ≈ 5.20 years = 3√3 years (since 3√3 ≈ 5.196). Equivalently: (1/3)^(3/2) = 1/√27 = 1/(3√3), and 27 × 1/(3√3) = 27/(3√3) = 9/√3 = 3√3 (NCERT Class 11 Physics Chapter 7, page 129).
Why A is wrong: A is wrong because it assumes T ∝ a (linear): 27 × (1/3) = 9. Kepler's law gives T ∝ a^(3/2), so the factor is (1/3)^(3/2) = 1/(3√3), not 1/3.
Why C is wrong: C is wrong because it assumes T ∝ a² (or equivalently, divides by 3²= 9): 27/9 = 3. The correct exponent is 3/2, giving 27/(3√3) = 3√3 ≈ 5.2 years.
Why D is wrong: D is wrong because it assumes T ∝ a³: 27 × (1/3)³ = 1. That would mean T² ∝ a⁶, not T² ∝ a³. The correct result is 3√3 years.
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Kepler's Laws: quick recall before you leave
How do you solve a Kepler's Laws question? A worked example
- 1
Given
• Satellite 1: semi-major axis a₁ = 2R, period T₁• Satellite 2: semi-major axis a₂ = 8R• Both orbit Earth (same central mass)
- 2
Required
Period T₂ of the second satellite.
- 3
Concept
Kepler's third law: for orbits around the same central body, T² ∝ a³.
- 4
Formula
T₂²/T₁² = (a₂/a₁)³
- 5
Substitution
T₂²/T₁² = (8R / 2R)³ = 4³ = 64
- 6
Calculation
T₂² = 64 T₁²
T₂ = 8 T₁
Note on exact values: The ratio a₂/a₁ = 8R/2R = 4 is an exact integer (the R cancels). The number 4 and the exponent 3/2 are exact mathematical quantities — they do not limit significant figures. - 7
Final answer
T₂ = 8 T₁
The second satellite's period is exactly 8 times the first. - 8
Common trap
A student who treats T as proportional to a (linear scaling) would compute T₂ = 4 T₁. This is the standard wrong answer in NEET. The correct power is 3/2: T₂/T₁ = 4^(3/2) = (√4)³ = 2³ = 8.
- 9
Similar NEET-style question
"Two planets orbit the same star. Planet A has semi-major axis a and period 10 years. Planet B has semi-major axis 9a. Find the period of planet B."
Answer: T_B = 10 × 9^(3/2) = 10 × 27 = 270 years.
---
What to remember before solving Kepler's Laws questions
Which Kepler's Laws formulas do you need for NEET?
1 formula — click to collapse
Kepler's third law
Square of orbital period proportional to cube of semi-major axis. Holds for elliptic orbits about a central mass.
| Symbol | Quantity | SI Unit |
|---|---|---|
| T | orbital period | s |
| a | semi-major axis | m |
| M | central mass | kg |
Valid when
- Two-body system with central mass M >> orbiting mass
- Bound orbit
Where do students lose marks on Kepler's Laws?
These are the exact patterns that cause wrong answers in NEET. Each trap includes when it triggers and how to avoid it.
2 items — click to collapse
Category: Similar Terms
Student treats T proportional to a (linear) instead of a^(3/2).
When it triggers
Question gives change in semi-major axis and asks for new period.
How to avoid
T² ∝ a³, so T ∝ a^(3/2). Doubling a multiplies T by 2^(3/2) ≈ 2.83.
Root cause: formula misuse
Correction
T² ∝ a³, so T ∝ a^(3/2). Doubling a multiplies T by 2^(3/2) ≈ 2.83. Quadrupling a → 8× T.
More in Gravitation: 2 exam traps and mistakes · 7 formulas · 3 question patterns from its other lessons.
Kepler's Laws questions from past NEET papers
2 questions from NEET 2025, 2026. Answers verified against NTA official keys. — click to collapse
How does NEET ask about Kepler's Laws?
1 recurring pattern from past papers — click to collapse
Given period T and semi-major axis a of one planet, find for another with different a. T^2 ∝ a^3.
Common distractors
uses linear relation
Treats T proportional to a not a^(3/2)
Sources
Page numbers are the ones printed in the current NCERT textbook (2023 rationalised edition), unless marked pre-2023. The books are free at ncert.nic.in.
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