Formula of Gravitation:

The formula of gravitation is given by Newton's law of gravitation which states that any two objects in the universe attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

The formula is:

F = G * (m1 * m2) / r^2

where F is the force of attraction between two objects, m1 and m2 are the masses of the two objects, r is the distance between their centers of mass, and G is the gravitational constant which has a value of 6.67 x 10^-11 Nm^2/kg^2.

Explanation:

The formula of gravitation is derived from the law of universal gravitation which states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

This means that the force of attraction between two objects decreases as the distance between them increases and increases as their masses increase. The constant G is a proportionality constant that depends on the units used to measure mass and distance.

The formula can be used to calculate the force of gravity between any two objects in the universe, from the attraction between two atoms to the attraction between planets and stars.

Conclusion:

In conclusion, the formula of gravitation is an important concept in physics that helps us understand the forces that govern the motion of objects in the universe. It is a simple yet powerful formula that has been used for centuries to study the behavior of celestial bodies and has led to many discoveries about the nature of the universe.