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The summary highlights the definition of gravitation as the attractive force between objects with mass, which governs the motion of celestial bodies and other physical phenomena. It explains the historical development of theories and concepts related to gravitation, including early ideas proposed by ancient civilizations and the significant contributions made by Isaac Newton and Albert Einstein. The page also delves into the mathematical formulas and laws associated with gravitation, such as Newton's law of universal gravitation and the general theory of relativity. The summary concludes by discussing gravitation in the context of astrophysics and cosmology, exploring its role in the formation and behavior of galaxies, stars, and the universe as a whole.