Newton and His Three LawsIsaac Newton's story of how an apple falling from a tree that hit his head inspired him to formulate a theory of Gravitation is a story that every schoolchild grows up hearing about. . Newton is arguably one of the most influential scientific minds in human history. He published books such as Arithmetica Universalis, The Chronology of Ancient Kingdoms, Methods of Fluxions, Opticks, the Queries and, most famously, Philosophiæ Naturalis Principia Mathematica. He formulated the three laws of gravitation, discovered the generalized binomial theorem, developed the calculus (credited to Gottfried Wilhelm Von Leibniz, who developed the theory independently), and worked extensively on optics and refraction of light. Newton changed the way people look at the world they live in and the way the universe works. Sir Isaac Newton was born on Christmas Day, December 25, 1642, based on the Julian calendar (4). January 1643, Gregorian calendar) at Woolsthorpe Manor in Woolsthorpe-by-Colsterworth, three months after his father's death. He was born prematurely and his mother Hannah Ayscough reportedly said he was small enough to fit in a cup. liter. Newton's mother remarried when he was three years old and left him in the care of his grandmother. This incident created a great deal of emotional distance between the scientist and his mother, and on top of that, Newton also admitted to scaring his parents by threatening to burn them and their house down. Another sad aspect of Newton's personal life is that although he was engaged, he never married. Newton was educated at the King's School in Grantham from the age of twelve to seventeen where he only learned Latin and not mathematics. Its mother is in the middle of paper...... each individual considers the Earth as a particle to do the analysis based on its orbital movement around a star. Here mass, acceleration, momentum and force are the externally defined quantities, that is, they are the externally defined quantities. It is also true that Newton's laws of motion are not sufficient to characterize the motion of deformable and rigid bodies. After the laws of motion proposed by Newton were generalized in 1950 by Leonhard Euler, the laws were also accepted for rigid bodies, and this was later called Euler's laws of motion. This theory was later applied to deformable bodies, and the laws were also true in this condition. Even though this law is overcome by the laws of relativity, this law is also applicable in situations where the speed of objects is less than the speed at which light travels..