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Gravitational Force

Reference from the original Physics I textbook.

Gravitational Force

The gravitational force between ordinary masses is attractive and acts along the line joining them. For point masses its magnitude is F = Gm₁m₂/r².

Related Glossary Terms

Gravitational Force Equation

Index

Chapter 3 - Gravity in Depth

Chapter 3 - FFR - Kepler’s Laws

Reviewed physics notes (1)

These corrections keep the original lesson’s purpose while fixing errors in the source edition.

  • Newtonian gravity does not repel ordinary positive masses. — Reference 1

About this edition and its source ↗

Glossary and deeper reading · 1 refreshers

These editorial refreshers supplement the reading. Definitions and examples are added guidance; original source wording and recorded answers remain in their original context.

  • Gravity

    Gravity is the attractive interaction between masses in the Newtonian model. For spherical bodies or point-mass approximations, its strength decreases with the square of the separation between their centers. For example, Earth’s gravity provides the inward force that keeps a satellite in orbit.

    Read more: Gravitational force →

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