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AP Physics 1 · Unit 2, Part 2 · Circular Motion and Gravity

Newton’s Law of Gravitation and Gravitational Fields

Change two masses and their separation to test gravitational force, then distinguish the force on an object from gravitational field strength.

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Newton’s Law of Gravitation and Gravitational Fields guided lesson preview Start guided lesson
Explore the model. Make predictions. Check your thinking.

Learn by doing

Three ideas you’ll put into motion

Compare masses

Predict how changing either mass changes the gravitational attraction.

Test the distance rule

Compare center-to-center separations to investigate the inverse-square relationship.

Separate force and field

Connect gravitational force with the force per unit test mass.

The big idea

The key ideas, at a glance.

Gravity depends on both masses

Newton’s law gives F = GMm/r2, where r is the separation between centers for point or spherically symmetric masses.

A field describes the source

Field strength is g = F/m = GM/r2. Changing the test mass changes force but not the source’s field.

A quick comparison

Double the separation while keeping both masses fixed.

Gravitational force becomes one quarter as large.

separation rseparation 2rSame masses → one quarter the force
Teaching this topic?Classroom fit, AP connections, and support
Classroom fit
Use for a concept introduction, guided independent practice, or a projected class discussion.
Before students begin
Newton’s laws, ratios, and squared quantities. Distinguish source mass from test mass.
Built-in support
Prepared scenes, guided prompts, and feedback on lesson questions.
AP Physics 1 connections
Unit 2: gravitational interactions, fields, and proportional reasoning.
Check for understanding
Ask what happens to force and field strength when only the test mass doubles.
Optional extension
Investigate the setup in the Newton’s Cannon experiment.
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