Skip to main content
Dr. Shreyank Educare
Curriculum-aligned learning support — not an official school, university, or ministry-approved course, and not a replacement for official credit.
Unit 3Lesson navigation

Physics 12 · Physics · Lesson 3.2

Gravitation

Level
Grade 12
Reading time
13 min reading
Review
Last reviewed 2026-09-03
Errata

Abstract

Newton's law of gravity.

What is Newton’s law of universal gravitation?

Short answer

Newton’s law of universal gravitation states that every mass attracts every other mass with a force proportional to the product of their masses and inversely proportional to the square of the distance between them: F = Gm₁m₂/r². G is the gravitational constant. This single law explains falling objects, the Moon’s orbit, and the motion of planets.

Concept preview

What you will be able to do

  1. 01Apply the universal law of gravitation F=Gm1m2/r2F = Gm_1m_2/r^2
  2. 02Relate gravitational field strength gg to mass and radius
  3. 03Use the inverse-square law to compare gravitational forces

Newton's leap of genius was realising that the force pulling an apple to the ground is the very same force keeping the Moon in orbit — gravity reaches across space. His law of universal gravitation states that every mass attracts every other mass with a force F=Gm1m2r2F = \dfrac{G m_1 m_2}{r^{2}}, where G=6.67×10−11 N⋅m2/kg2G = 6.67\times10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2 is the universal gravitational constant and rr is the distance between the centres. Bigger masses pull harder; greater distance pulls weaker.

School Plan

Gravitation

This lesson's full explanation, worked examples, quiz and practice are locked. Full access is on the School Plan.

Log in or start free and you will return right here.

Related topics

Frequently asked questions

What does "inverse-square" mean here?
Doubling the distance between two masses reduces the gravitational force to a quarter of its value.
Why don’t we feel gravity between everyday objects?
G is extremely small, so gravitational forces are only noticeable when at least one mass is very large, like a planet.