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SSC CGL - Detailed Guide 2025

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Gravitation

Reference: Lucent GK, NCERT Class 6–12

1. Universal Law of Gravitation

Proposed by Sir Isaac Newton.

Every object in the universe attracts every other object with a force that is:

  • Directly proportional to the product of their masses.
  • Inversely proportional to the square of the distance between them.

F = G × (m₁ × m₂) / r²

Newton's Universal Law of Gravitation
Symbol Meaning SI Unit
F Gravitational force newton (N)
G Universal Gravitational Constant 6.674 × 10⁻¹¹ Nm²/kg²
m₁, m₂ Masses of the two objects kilograms (kg)
r Distance between objects meters (m)
  • G is a universal constant, same throughout the universe.
  • This law explains motion of planets, tides, satellite orbits, etc.
Illustration of accelerate due to Gravity

2. Acceleration due to Gravity (g)

When objects fall freely under gravity, they accelerate at a constant rate called acceleration due to gravity.

g = G × (M / R²)

Quantity Symbol Value on Earth Unit
Acceleration due to gravity g 9.8 m/s²
Mass of Earth M 5.972 × 10²⁴ kg
Radius of Earth R 6.371 × 10⁶ m

g decreases:

  • With altitude
  • With depth (toward Earth's center)
  • At equator compared to poles
  • g = 0 at the center of Earth

3. Mass vs. Weight

Factor Mass Weight
Definition Amount of matter in body Force with which Earth attracts
Symbol m W
Formula m = Density × Volume (m = ρV) ; m = Weight / Gravitational Acceleration(m = W/g) ; m = Force / Acceleration (m = F/a) ; m = Energy / (Speed of Light)² (m = E/c²) W = m × g
Nature Scalar Vector
Unit kg newton (N)
Constant? Yes (anywhere in universe) No (depends on gravity)
Measured by Beam balance Spring balance

Note: Weight is zero in space (g = 0), but mass remains constant.

4. Free Fall

When an object falls under the influence of gravity alone (no air resistance), it is in free fall.

Equations of motion apply with:

  • Initial velocity (u) = 0
  • Acceleration = g = 9.8 m/s² (downward)
 Illustration of Free Fall Motion
Equation Description
v = gt Velocity after time t
s = ½gt² Distance fallen in time t
v² = 2gs Velocity after falling a distance s

Note: In vacuum, all objects fall at same rate regardless of mass.

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