THEORY OF GRAVITATION Meaning and
Definition
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The theory of gravitation, also known as the theory of gravity, is a fundamental scientific explanation for the force that governs the movement and interactions of massive bodies. It postulates that the force of gravity arises due to the mass of an object, and it is a universal force acting between all objects with mass. This overarching theory was first proposed by Sir Isaac Newton in the late 17th century, and later refined by Albert Einstein's general relativity theory in the early 20th century.
According to the theory of gravitation, any two objects in the universe exert an attractive force on each other, and the strength of this force is proportional to the product of their masses and inversely proportional to the square of the distance between their centers. It describes how objects with mass are influenced by gravity, causing them to be drawn towards one another. The theory explains why objects fall to the ground when released, how celestial bodies like planets orbit around the Sun, and even extends to the behavior of galaxies in the vast expanse of the universe.
The theory of gravitation revolutionized our understanding of the cosmos and paved the way for numerous scientific advancements and space exploration. It has been extensively proven through experimental observations and mathematical calculations and remains one of the cornerstones of modern physics.
Common Misspellings for THEORY OF GRAVITATION
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