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Gravitation

Universal gravitation, orbital motion, escape velocity

Key Concepts

  • Kepler's 1st law: planets move in ellipses with sun at one focus
  • Kepler's 2nd law: equal areas are swept in equal times (L conserved)
  • Kepler's 3rd law: T² ∝ r³
  • Gravitational field is zero at centre of a uniform spherical shell
  • g decreases both above and below Earth's surface

Important Formulae

Gravitational force F = Gm₁m₂/r²
Surface gravity g = GM/R²
Escape velocity v_esc = √(2GM/R) = √(2gR)
Orbital velocity v_orb = √(GM/r)
Orbital period T = 2πr/v_orb
g at height h g_h = g(1 − 2h/R) for h ≪ R

Quick Tips

  • Escape velocity ≈ 11.2 km/s for Earth; orbital velocity for near-orbit ≈ 7.9 km/s.
  • Geostationary orbit: T = 24 h, height ≈ 36,000 km above equator.
  • Gravitational PE = −GMm/r (negative because bound system).

Sample Practice Questions

  1. Kepler's second law states that the line joining planet and sun sweeps equal areas in:

    • Proportional distances
    • Equal time intervals
    • Proportional time intervals
    • Equal distances
    Show answer

    Answer: Equal time intervals

  2. The gravitational potential at Earth's centre (surface potential = V₀):

    • -V₀/2
    • -V₀
    • -3V₀/2
    • -2V₀
    Show answer

    Answer: -3V₀/2

  3. A satellite in circular orbit has total energy:

    • GMm/2r
    • -GMm/2r
    • GMm/r
    • -GMm/r
    Show answer

    Answer: -GMm/2r

  4. Intensity of gravitational field at a point is:

    • Force per unit volume
    • Force per unit mass
    • Force × mass
    • Force × distance
    Show answer

    Answer: Force per unit mass

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Practice Questions

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Frequently Asked Questions

What are the key concepts in Gravitation for NEET?

Kepler's 1st law: planets move in ellipses with sun at one focus; Kepler's 2nd law: equal areas are swept in equal times (L conserved); Kepler's 3rd law: T² ∝ r³; Gravitational field is zero at centre of a uniform spherical shell; g decreases both above and below Earth's surface.

Which formulae are important for Gravitation in NEET?

Gravitational force: F = Gm₁m₂/r²; Surface gravity: g = GM/R²; Escape velocity: v_esc = √(2GM/R) = √(2gR); Orbital velocity: v_orb = √(GM/r); Orbital period: T = 2πr/v_orb; g at height h: g_h = g(1 − 2h/R) for h ≪ R.

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