NEET · Physics

NEET Gravitation: g, Potential, Escape Velocity and Satellites

Own the complete official Unit 6 Gravitation intent: universal law, variation of g, Kepler laws, potential/potential energy, escape velocity, circular satellite motion, orbital velocity, time period and satellite energy.

Subject
Physics
Official syllabus unit
Unit 6: Gravitation

In short

Gravitation is the single canonical Rank Sarthi owner for official Unit 6. Use inverse-square force outside a spherically symmetric mass, distinguish gravitational potential from potential energy, and apply satellite/escape formulas only under the central spherical-body and idealized orbit conditions stated with each relation.

Subject faculty

Ashwini M., Physics Expert at Rank Sarthi

Ashwini M.

Physics Expert

Physics • NEET

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Also in Physics: Kumar Gandharva Saxena

Syllabus mapping

  • Unit
    Current official NEET UG 2026 scope
    Topics
    Universal gravitation and spherical bodies, Potential vs potential energy, Satellites, Escape

Before this chapter

Concepts in this chapter

1. Universal gravitation and spherical bodies

For point masses, gravitational force follows the inverse-square law along the line joining them. For a spherically symmetric body, the external field behaves as if the mass were concentrated at the center. Inside a real Earth, simple depth formulas require model assumptions about density; the common linear g with depth result assumes uniform density.

2. Potential vs potential energy

Gravitational potential is energy per unit test mass and is a scalar. With zero potential at infinity, potential outside a spherical mass is negative: V=-GM/r. Potential energy of a mass m is U=mV=-GMm/r.

3. Satellites

Circular-orbit formulas require a circular orbit around a dominant central mass, with other interactions neglected. Orbital speed and period depend on orbital radius measured from the central body's center, not height above the surface unless radius is first converted.

4. Escape

Escape speed is obtained by the minimum-energy condition for reaching infinity with zero residual speed in the ideal central-field model. It is not the same as orbital speed; at the same radius, v_escape = sqrt(2) v_orbit for the standard spherical central-mass model.

5. Decision aids for this chapter

  • Potential vs potential-energy comparison card
  • Orbit radius vs altitude diagram
  • g-variation assumptions panel

Formula sheet

  • Universal law: F = G m1 m2 / r^2. Magnitude; N. Point masses or external field of spherical masses; force is attractive along line joining centers.

    Universal law

    Use when — Magnitude; N. Point masses or external field of spherical masses; force is attractive along line joining centers.

  • Surface/outside gravity: g = GM/r^2. m s^-2. Outside spherical mass or at surface r=R; direction inward.

    Surface/outside gravity

    Use when — m s^-2. Outside spherical mass or at surface r=R; direction inward.

  • Altitude variation: g_h = g_0 [R/(R+h)]^2. Spherical-body model; h measured above surface.

    Altitude variation

    Use when — Spherical-body model; h measured above surface.

  • Depth variation, uniform density: g_d = g_0(1-d/R). Requires uniform-density spherical Earth model; d depth below surface. Do not present as exact for real Earth.

    Depth variation, uniform density

    Use when — Requires uniform-density spherical Earth model; d depth below surface. Do not present as exact for real Earth.

  • Potential: V = -GM/r. Scalar; J kg^-1 = m^2 s^-2. Zero chosen at infinity.

    Potential

    Use when — Scalar; J kg^-1 = m^2 s^-2. Zero chosen at infinity.

  • Potential energy: U = -GMm/r. Scalar; J. Same zero-at-infinity convention.

    Potential energy

    Use when — Scalar; J. Same zero-at-infinity convention.

  • Circular orbital speed: v_o = sqrt(GM/r). Circular orbit about dominant spherical central mass; r from center.

    Circular orbital speed

    Use when — Circular orbit about dominant spherical central mass; r from center.

  • Circular orbital period: T = 2π sqrt(r^3/GM). Circular orbit; gives Kepler T^2 ∝ r^3 for same central mass.

    Circular orbital period

    Use when — Circular orbit; gives Kepler T^2 ∝ r^3 for same central mass.

  • Escape speed: v_e = sqrt(2GM/r). Minimum launch speed in ideal central field neglecting atmosphere/rotation; from radius r.

    Escape speed

    Use when — Minimum launch speed in ideal central field neglecting atmosphere/rotation; from radius r.

  • Circular-orbit total energy: E = -GMm/(2r). Circular orbit under Newtonian gravity around dominant central mass.

    Circular-orbit total energy

    Use when — Circular orbit under Newtonian gravity around dominant central mass.

Worked examples

At some radius from a spherical planet, the circular orbital speed is 4.0 km s^-1. What is the ideal escape speed from the same radius?

Concept being tested: Escape vs orbit

Prompt: At some radius from a spherical planet, the circular orbital speed is 4.0 km s^-1. What is the ideal escape speed from the same radius?

Decisive condition: Same radius and same central-field model; use the exact relation v_e=sqrt(2)v_o.

Method choice: Multiply the circular orbital speed by sqrt(2).

Reasoning/calculation: v_e≈1.414×4.0=5.66 km s^-1.

Unit/sign/condition check: Both are speeds in km s^-1. The relation assumes the same radius and ideal central Newtonian field.

PI if answered incorrectly: Recall Gap if the relation is forgotten; Decision / Selection Error if values from different radii are compared directly.

Common mistakes and what they actually indicate

  • Using height h directly as orbital radius

    Execution error

    Why it happens

    Preparation Intelligence classification: Execution Error.

    How it is corrected

    Use r=R+h from the center.

  • Confusing potential V with potential energy U

    Knowledge gap

    Why it happens

    Preparation Intelligence classification: Knowledge Gap.

    How it is corrected

    Remember U=mV.

  • Using linear depth formula without the uniform-density assumption

    Decision / selection error

    Why it happens

    Preparation Intelligence classification: Decision / Selection Error.

    How it is corrected

    State the model assumption or use a more appropriate model.

  • Treating escape speed as orbital speed

    Recall gap

    Why it happens

    Preparation Intelligence classification: Recall Gap.

    How it is corrected

    At the same radius in the ideal model, v_e=sqrt(2)v_o.

FAQ

NEET Gravitation: g, Potential, Escape Velocity and Satellites — questions

Straight answers about how Rank Sarthi fits into serious exam preparation.

/neet/physics/gravitation.

Sources and provenance

Official scope is taken from the NEET (UG) 2026 syllabus and official NTA documents; concept structure follows current NCERT contents. No performance, weightage or question-frequency data is asserted.