Authors:
Newton’s laws of gravitation, proposed about three to four decades ago, are still widely used in most fields of modern physics. Although the gravitational equation put forward by Newton, [F = Gm1m2/r2] (where F represents the force, m1 and m2 are the masses of the interacting objects, r is the distance between the two objects, and G is the gravitational constant), is purely empirical; it eventually took the form of a law. In fact, it was an intuitive equation formulated by Newton based on his observations of various natural phenomena, such as the falling of an apple from a tree, the motion of planets in the solar system, the Earth's rotation on its axis, and the periodic tides in rivers and oceans. Newton believed that his proposed equation (or the gravitational model as he envisioned it) was the best fit for the experimental data available at the time. This data included the relationship between the height and time of an object's fall towards the Earth, the symmetry of an object's time of ascent and descent, and the escape velocity required for an object to leave Earth's gravitational influence. However, in formulating his law, Newton entirely ignored or overlooked four fundamental aspects of the universe: Thermodynamics, The perpetual motion phenomena, The cancellation of the g parameter between the ‘acceleration parameter’ and ‘time’ in his proposed equations and the ‘time temperature’ entanglement of the universe. So, this paper relooked at classical physics with these four above fundamental aspects of the universe and presented new outputs.
Keywords: Newton’s Laws of Gravitation; Modern Physics; Solar System; Time Temperature
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