Basics of Gravitational Fields

4. Inverse-Square Law

Learning Outcomes
  • I can explain the inverse-square relationship in gravitation.
  • I can predict how gravitational force changes with distance.
  • I can calculate force changes when distance is doubled or halved.
  • I can interpret graphs showing inverse-square relationships.
  • I can apply the inverse-square law to planetary and satellite systems.

Key Topics:
  • Inverse-square law derivation
  • Gravitational field examples

What is the Inverse-Square Law?

One of the most important features of gravity is that its strength decreases rapidly as the distance between two objects increases.

This relationship is called the inverse-square law.

The inverse-square law states:

The gravitational force between two objects is inversely proportional to the square of the distance between their centres.

This means that even a small increase in distance can produce a large decrease in gravitational force.


The Mathematics of the Inverse-Square Law

Newton's Law of Universal Gravitation is:

 
F=Gm1m2r2F = G \frac{m_1 m_2}{r^2}
F=G(8)(8)(14)2=21.8 NF=G\frac{(\text{8})(\text{8})}{(\text{14})^2}=\text{21.8}\,\mathrm{N}
The force grows with both masses and shrinks quickly as distance increases.
m1m_1m1​
kg
 
m2m_2m2​
kg
 
rrr
m
 
F=21.8F = \text{21.8}F=21.8F = \text{21.8}m_18m_28r=14r = \text{14}

Notice that the distance r appears in the denominator as r².

This means:

F∝1r2F\propto\frac{1}{r^2}

The force does not decrease in direct proportion to distance—it decreases with the square of the distance.


How Distance Affects Gravity

Suppose the distance between two objects changes while their masses remain constant.

If the distance doubles

r→2rr\rightarrow2r

The force becomes:

122=14\frac{1}{2^2} = \frac14

The gravitational force becomes one-quarter of its original value.


If the distance triples

r→3rr\rightarrow3r

The force becomes:

19\frac1991​

Only one-ninth of the original force remains.


If the distance becomes four times larger

r→4rr\rightarrow4r

The force becomes:

116\frac1{16}161​

Only one-sixteenth of the original force remains.


If the distance is halved

r→12rr\rightarrow\frac12r

The force becomes:

4F4F4F

The gravitational force becomes four times stronger.


Summary Table

Change in Distance Change in Gravitational Force
Double (×2) 1/4 as large
Triple (×3) 1/9 as large
Four times farther (×4) 1/16 as large
Half (×1/2) 4 times larger
One-third (×1/3) 9 times larger

This demonstrates how strongly gravity depends on distance.


Why Does Gravity Decrease So Quickly?

Imagine a light bulb shining equally in all directions.

As you move farther away:

  • The same amount of light spreads over a larger area.
  • The light appears dimmer.

Gravity behaves in a similar way.

As the distance increases, the gravitational influence spreads over a larger spherical area.

Since the surface area of a sphere increases as:

A=4πr2A=4\pi r^2

the strength of gravity decreases with the square of the distance.


Worked Example 1

Two planets exert a gravitational force of 800 N on each other.

If the distance between them doubles, what is the new force?

Step 1

Doubling the distance gives:

14\frac1441​

of the original force.

Step 2

Calculate:

800×14=200 N800\times\frac14=200\text{ N}

Answer

200 N\boxed{200\text{ N}}200 N​

Worked Example 2

A satellite experiences a gravitational force of 120 N.

It moves to half its original distance from Earth.

What is the new force?

Step 1

Halving the distance increases the force by:

444

Step 2

Calculate:

120×4=480 N120\times4=480\text{ N}

Answer

480 N\boxed{480\text{ N}}480 N​

Interpreting Graphs

A graph of gravitational force against distance has a distinctive shape.

It is not a straight line.

Instead:

  • The force decreases rapidly at small distances.
  • The curve gradually flattens as distance increases.
  • The graph approaches zero but never actually reaches it.

This type of curve is called an inverse-square curve.

Unlike a linear graph, equal increases in distance do not produce equal decreases in force.


Inverse-square relationship

Relative gravitational force decreases rapidly as distance increases according to the inverse-square law.

 
00.30.60.91.21r2r3r4r5r

Applications in the Solar System

The inverse-square law explains why:

Planets farther from the Sun experience weaker gravity.

For example:

  • Mercury experiences a much stronger gravitational pull from the Sun than Neptune.

Satellites

As a satellite moves farther from Earth:

  • Earth's gravitational pull decreases.
  • The satellite moves more slowly in its orbit.

This is why satellites in higher orbits take longer to complete one revolution.


Moons

The same law explains why moons orbiting far from their planets experience weaker gravitational forces than nearby moons.


Why the Inverse-Square Law Matters

Scientists use the inverse-square law to:

  • Predict planetary orbits.
  • Calculate satellite trajectories.
  • Design space missions.
  • Study binary star systems.
  • Understand galaxy interactions.

Without the inverse-square law, modern astronomy and space exploration would not be possible.


Common Mistakes

Students often confuse an inverse relationship with an inverse-square relationship.

Incorrect thinking

"If the distance doubles, the force halves."

❌ This is wrong.


Correct thinking

"If the distance doubles, the force becomes one-quarter."

✔ Because the distance is squared.

Always remember:

Square the distance first.


Key Terms

Inverse-Square Law — A relationship in which a quantity decreases in proportion to the square of the distance.

Inverse Proportion — A relationship in which one quantity decreases as another increases.

Relative Force — The force expressed as a fraction or multiple of another force.


Key Takeaways

  • Gravitational force follows the inverse-square law.
  • Doubling the distance reduces the force to one-quarter.
  • Halving the distance increases the force by four times.
  • The inverse-square law produces a curved graph rather than a straight line.
  • This relationship explains the motion of planets, moons, and satellites.
  • The inverse-square law is fundamental to astronomy, astrophysics, and space exploration.

Suggested Images

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Suggested placement:

  1. After "How Distance Affects Gravity" – Diagram comparing two masses at distances r, 2r, and 3r, with arrows showing the decreasing gravitational force.
  2. After "Why Does Gravity Decrease So Quickly?" – Illustration of expanding spheres (or light spreading from a bulb) to visualize why intensity and gravitational influence decrease withr2r^2r2.
  3. After "Applications in the Solar System" – Diagram of the Solar System highlighting that planets farther from the Sun experience weaker gravitational attraction.
  4. After "Satellites" – Comparison of a low-Earth orbit satellite and a high-altitude satellite, illustrating weaker gravity and longer orbital periods at greater distances.