KAHIBARO
Table of Contents
A Universal Attraction
Universal gravitation is the idea that every object with mass attracts every other object with mass. This attraction is not limited to objects on Earth. It acts between apples and Earth, between Earth and the Moon, between planets and the Sun, and between stars and galaxies. The word universal means that the same rule applies everywhere.
Before Newton, people often thought that falling objects on Earth and the motion of planets in the sky were different kinds of phenomena. Newton showed that they can be understood by one single law. The same gravitational interaction that pulls a stone downward also keeps the Moon in orbit around Earth.
Newton's Law of Universal Gravitation
Newton proposed that the gravitational force between two point masses depends on their masses and the distance between them. The force is stronger when the masses are larger, and weaker when the distance is greater.
The law is
$$
F = G \frac{m_1 m_2}{r^2}
$$
where $F$ is the magnitude of the gravitational force, $m_1$ and $m_2$ are the two masses, $r$ is the distance between their centers, and $G$ is the gravitational constant.
For two masses $m_1$ and $m_2$ separated by distance $r$,
$$
F = G \frac{m_1 m_2}{r^2}
$$
This force is always attractive.
This equation is called an inverse square law because the force varies as $\frac{1}{r^2}$. If the distance doubles, the force becomes one fourth as large. If the distance triples, the force becomes one ninth as large.
Meaning of the Formula
Each part of the equation has a clear physical meaning. The product $m_1 m_2$ shows that both masses matter. If one mass doubles, the force doubles. If both masses double, the force becomes four times larger.
The factor $r^2$ in the denominator shows that distance reduces the force quickly. This is why the gravitational attraction between everyday objects is usually extremely small, while the attraction between planets and stars is large enough to control their motion.
The constant $G$ sets the overall strength of gravity in nature. Its value is small, which tells us that gravity is much weaker than many other forces when we deal with small objects.
Direction of the Force
Gravity is not only a number, it is a force with direction. The gravitational force acts along the line joining the centers of the two masses. Each object pulls the other toward itself.
If object 1 pulls object 2 with force $\vec{F}_{12}$, then object 2 pulls object 1 with force $\vec{F}_{21}$ of equal magnitude and opposite direction. This matches Newton's third law.
Gravitational forces between two objects always come in pairs. They have equal magnitude, opposite direction, and act on different objects.
Point Masses and Spherical Bodies
The formula is exact for point masses. A point mass is an object whose size is very small compared with the distance involved, or an ideal object treated as if all its mass were concentrated at one point.
For many real objects, especially spheres, the same formula can still be used if the bodies are spherically symmetric. Then the object behaves as if all its mass were concentrated at its center. This is why we often calculate the gravitational force between Earth and the Moon by using the distance between their centers.
How the Force Changes with Distance
The inverse square dependence is one of the most important features of gravitation. It leads to simple comparison rules.
Suppose the original force is
$$
F_0 = G \frac{m_1 m_2}{r^2}
$$
If the new distance is $kr$, then the new force is
$$
F = G \frac{m_1 m_2}{(kr)^2} = \frac{F_0}{k^2}
$$
The table below shows some examples.
| Change in distance | New force |
|---|---|
| $r \to 2r$ | $F \to \frac{F_0}{4}$ |
| $r \to 3r$ | $F \to \frac{F_0}{9}$ |
| $r \to \frac{r}{2}$ | $F \to 4F_0$ |
| $r \to \frac{r}{3}$ | $F \to 9F_0$ |
This strong dependence on distance explains why gravity from very distant objects becomes weak, even if those objects are massive.
How the Force Changes with Mass
The force is directly proportional to each mass. If one mass changes by a factor, the force changes by the same factor.
| Change in mass | New force |
|---|---|
| $m_1 \to 2m_1$ | $F \to 2F_0$ |
| $m_2 \to 3m_2$ | $F \to 3F_0$ |
| $m_1 \to 2m_1$, $m_2 \to 2m_2$ | $F \to 4F_0$ |
This tells us that larger bodies exert stronger gravitational pulls.
A Simple Example
Consider two masses, $m_1 = 2\,\text{kg}$ and $m_2 = 3\,\text{kg}$, separated by $r = 1\,\text{m}$. Then
$$
F = G \frac{(2)(3)}{1^2} = 6G
$$
Since $G$ is very small, the force is also very small. This shows why gravity between ordinary objects in a room is hard to notice.
Now imagine one of the masses is Earth. Because Earth's mass is enormous, the gravitational force becomes significant.
Why Universal Gravitation Matters
Universal gravitation connects many physical situations with one law. It explains why objects fall, why moons orbit planets, why planets orbit stars, and why large astronomical systems hold together.
Its importance is not only that gravity exists, but that the same mathematical law applies everywhere. This universality is one of the deepest ideas in physics.
Visualizing the Attraction
The two objects pull each other along the line joining their centers.
Key Ideas to Remember
Universal gravitation says that every mass attracts every other mass. The force depends on the product of the masses and decreases with the square of the distance between them. It is always attractive and acts along the line joining the two masses.
Gravity is universal, attractive, and follows the inverse square law:
$$
F = G \frac{m_1 m_2}{r^2}
$$
Larger masses give stronger attraction. Greater distance gives weaker attraction.