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Isaac Newton's Universal Law of Gravitation states that all objects in the universe, regardless of their size, exert a gravitational force on each other. This force is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. The law explains various gravitational phenomena observed in the solar system and beyond.
The Universal Law of Gravitation, formulated by Isaac Newton, describes the foundational principles of gravitational interaction in the universe. It asserts that:
F = G (M × m) / d² where G is the universal gravitational constant. - The law is applicable universally, affecting both celestial bodies like planets and moons and terrestrial objects.
The significance of this law extends to explaining remarkable phenomena, such as the orbital motion of planets around the Sun, the attraction between the Earth and the Moon, and the condition of floating objects in fluids due to buoyancy, all fundamentally rooted in gravitational interactions. Understanding this law provides a basis for exploring more complex concepts in astrophysics and mechanics.
Gravitational force is universal: It acts between all objects with mass.
The strength of gravity depends on the mass of the objects and the distance between them.
The formula for gravity (F = G (M × m) / d²) describes how force is calculated.
Gravity's pull is far and wide, all things near and far collide.
Once upon a time, gravity threw a party where every object from the tiniest atom to the largest planet was invited. They all attracted each other and danced around, reminding one another of Newton's everlasting rules.
G = Gravitational constant, M = Mass 1, m = Mass 2, d = Distance squared. Remember: 'Get More Mass, Divide'.
Illustration of gravitational pull: The Earth attracts an apple, causing it to fall, which is a direct observation of gravitational force.
The Moon's orbit around the Earth is maintained by gravitational forces acting between them, preventing it from drifting away.
Term: Gravitational Force
Definition: The force of attraction that exists between any two objects with mass.
The force of attraction that exists between any two objects with mass.
Term: Universal Law of Gravitation
Definition: A law stating that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
A law stating that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
Term: Gravitational Constant (G)
Definition: A proportionality constant used in the calculation of gravitational force, approximately equal to 6.674 × 10⁻¹¹ N m²/kg².
A proportionality constant used in the calculation of gravitational force, approximately equal to 6.674 × 10⁻¹¹ N m²/kg².
Term: Mass
Definition: The amount of matter in an object, usually measured in kilograms.
The amount of matter in an object, usually measured in kilograms.
Term: Distance (d)
Definition: The separation between the centers of two objects, which affects the strength of the gravitational force between them.
The separation between the centers of two objects, which affects the strength of the gravitational force between them.