F = G * (m1 * m2) / r²

Where:

* F is the gravitational force between two objects

* G is the gravitational constant (approximately 6.674 × 10⁻¹¹ N⋅m²/kg²)

* m1 is the mass of the first object

* m2 is the mass of the second object

* r is the distance between the centers of the two objects

Explanation:

* Gravitational force is the force of attraction between any two objects with mass.

* Gravitational constant (G) is a fundamental constant that determines the strength of the gravitational force.

* Mass is a measure of the amount of matter in an object.

* Distance is the separation between the centers of the two objects.

Key points:

* The force is proportional to the product of the masses. This means that the more massive the objects, the stronger the gravitational force between them.

* The force is inversely proportional to the square of the distance. This means that the farther apart the objects are, the weaker the gravitational force between them.

This formula describes the gravitational force between any two objects, from tiny particles to massive planets. It is a fundamental law of nature that governs the motion of celestial bodies and the structure of the universe.