Fundamental interaction affecting all matter.
Gravity is one of the four fundamental forces of nature, alongside electromagnetism, and the strong and weak nuclear forces. It is the force that attracts two objects towards each other. Everything that has mass also has gravity. Objects with more mass have more gravity, and gravity gets weaker with distance.
Sir Isaac Newton was the first to formulate a law describing gravity, which is now known as Newton's Law of Universal Gravitation. This law states that every particle of matter in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
Mathematically, this can be expressed as:
F = G * (m1 * m2 / r^2)
Where:
The gravitational constant (G) is a physical constant involved in the calculation of gravitational effects. It is an empirical physical constant involved in the calculation of gravitational force between two bodies. It appears in Newton's law of universal gravitation and in Einstein's theory of general relativity. It is approximately equal to 6.67430(15)×10^−11 N(m/kg)^2.
The inverse-square law of gravity is derived from Newton's law of universal gravitation. It states that the force of gravity acting between any two objects is inversely proportional to the square of the distance that separates them. This means that if the distance between two objects is doubled, the gravitational attraction between them is reduced to a quarter of its original value.
When there are more than two objects, the net gravitational force on a given object is simply the vector sum of the forces exerted on it by the other objects. Each force is calculated as if the other objects were not present.
In conclusion, understanding gravitational forces is fundamental to understanding the physical world around us. From the motion of planets in our solar system to the tides in our oceans, gravity plays a crucial role in shaping our universe.