LAW OF GRAVITATION Meaning and
Definition
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The law of gravitation is a fundamental scientific principle that describes the force of attraction between objects with mass. Proposed by Sir Isaac Newton in the late 17th century, the law of gravitation 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. It mathematically expresses the relationship between these factors as F = G × (m1 × m2) / r^2, where F represents the force of gravitation, G denotes the gravitational constant, m1 and m2 are the masses of the objects, and r stands for the distance separating them.
The law of gravitation elucidates the concept of gravity, the force that governs the motion and interactions of celestial bodies, including planets, stars, and galaxies. Gravity is responsible for keeping celestial objects in their respective orbits around larger bodies, such as planets revolving around the Sun. It is a universal force, operating on both macroscopic and microscopic scales, shaping the structure of the universe. For instance, gravity plays a pivotal role in determining the motion of tides on Earth and has a significant influence on the behavior of celestial objects, such as the formation and evolution of galaxies.
Newton's law of gravitation is considered one of the pillars of classical physics, providing a framework to understand and predict the dynamics of celestial bodies. However, this law was later modified by Albert Einstein's theory of general relativity to account for situations involving high gravitational fields or extreme speeds, where gravitational effects become more pronounced. Nevertheless, the law of gravitation remains a fundamental basis for comprehending the force that binds the cosmos together, shedding light on the intricate workings of the universe.
Common Misspellings for LAW OF GRAVITATION
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