Gravitational pull, also known as gravity, is the force of attraction that exists between any two masses in the universe. This force is what keeps planets in orbit around the sun, and what causes objects to fall to the ground when they are dropped. Gravitational pull is one of the four fundamental forces in the universe, and it is described by Isaac Newton's law of universal gravitation.
Key Concepts:
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.
Gravitational Force Equation: The gravitational force (F) between two objects can be calculated using the equation F = G * (m1 * m2) / r^2, where G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between their centers.