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He expressed this concept in his book Discorsi e dimostrazioni matematiche intorno a due nuove scienze attenenti alla meccanica or Dialogues Concerning Two New Sciences , in which he states:. It has been observed that missiles and projectiles describe a curved path of some sort; however no one has pointed out the fact that this path is a parabola.

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But this and other facts, not few in number or less worth knowing, I have succeeded in proving; and what I consider more important, there have been opened up to this vast and most excellent science, of which my work is merely the beginning, ways and means by which other minds more acute than mine will explore its remote corners. Those prophetic words would later be borne out by the work of Newton.

Perhaps of more immediate significance, however, was the fact that Galileo had found an answer to the problem arising from Copernicus' theories, namely the question of why an observer on Earth experiences no sensation of motion, despite the fact the Earth is supposedly moving through space at high speed and revolves around its axis. One of the arguments frequently made against the notion that the Earth was moving went something like this: If the Earth is moving, then surely a stone dropped from a tower should move away from the tower as it falls? Galileo could now argue that, since the stone must be moving in the same direction as the tower immediately before it is dropped, then it will continue to move in that direction unless some external force or entity prevents it from doing so.

Galileo later became even more convinced of the veracity of the heliocentric view of the solar system when the invention of the telescope in circa allowed him to look more closely at the motion of various objects in the night sky. Galileo's observations led him to the discovery of Jupiter's four largest moons which he at first thought were stars. After studying these objects for several weeks he concluded that they must be orbiting Jupiter just as, according to Copernicus, the planets of the solar system must orbit the Sun.

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Nevertheless, there was still a great deal of hostility towards the heliocentric view of the solar system, not least because it directly contradicted the official view of the Catholic church at the time, which was that the Earth was at the centre of the universe, and that the Sun, Moon and stars revolved around it. Indeed, Galileo's support of heliocentrism put him on a collision course with the church that eventually led to him being tried for heresy, and saw him forced to spend the last few years of his life under house arrest.

The Copernican view of the solar system was also endorsed by the German mathematician, astronomer, and astrologer Johannes Kepler , who was to become one of the key figures in the scientific revolution. Kepler learned of the Copernican system of planetary motion as a student, and became a dedicated supporter of Copernicus' ideas.

History of classical mechanics

Kepler had proved himself to be an outstanding mathematician, and when his studies ended he accepted a post teaching mathematics in Graz the second largest city in Austria. During Kepler's tenure in Gratz, and based on his knowledge of three-dimensional geometry, he gradually developed a working theory concerning the geometrical ordering of the planets in the solar system.

These ideas appeared in his first major astronomical work Mysterium Cosmographicum The Cosmographic Mystery , which was originally published in A greatly expanded edition, which included a number of corrections and improvements, was published in In In pursuance of his theories, Kepler sought the opinions of many other astronomers of the period. Brahe was renowned for his accurate and comprehensive astronomical and planetary observations. In , Kepler met with Brahe in Prague.

As a result of that meeting, he accepted a post as Brahe's assistant, and was assigned the task of analysing the observational data that Brahe provided. When Brahe died rather unexpectedly in , Kepler succeeded him as imperial mathematician. His brief was to complete Brahe's unfinished work, and to provide astrological services to the Emperor.

Kepler remained in Prague until , and spent those years analysing the extensive observational data that Brahe had gathered. It was in , towards the end of his tenure there, that Galileo discovered the moons of Jupiter.

From Copernicus to Newton

Galileo sought the opinion of Kepler on this matter, who was happy to lend his support to Galileo's findings and later published his own observations of Jupiter's moons. Kepler's work had a number of important outcomes. One of these was the Tabulae Rudolphinae Rudolphine Tables - a star catalogue and a set of planetary tables based on Brahe's observational data, named for the Emperor and eventually published by Kepler in If you apply a force to an empty shoebox sitting on a table, the shoebox applies an equal force back on you. Remember that according to the Second Law , force and acceleration are related but they aren't identical!

Because your mass is much larger than the mass of the shoebox, the force you exert causes it to accelerate away from you. The force it exerts on you wouldn't cause much acceleration at all. Not only that, but while it's pushing on the tip of your finger, your finger, in turn, pushes back into your body, and the rest of your body pushes back against the finger, and your body pushes on the chair or floor or both , all of which keeps your body from moving and allows you to keep your finger moving to continue the force.

There's nothing pushing back on the shoebox to stop it from moving. If, however, the shoebox is sitting next to a wall and you push it toward the wall, the shoebox will push on the wall and the wall will push back. The shoebox will, at this point, stop moving.

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  • You can try to push it harder, but the box will break before it goes through the wall because it isn't strong enough to handle that much force. Most people have played tug of war at some point. A person or group of people grab the ends of a rope and try to pull against the person or group at the other end, usually past some marker sometimes into a mud pit in really fun versions , thus proving that one of the groups is stronger than the other.

    All three of Newton's Laws can be seen in a tug of war. There frequently comes a point in a tug of war when neither side is moving.

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    Both sides are pulling with the same force. Therefore, the rope does not accelerate in either direction.

    This is a classic example of Newton's First Law. Once a net force is applied, such as when one group begins pulling a bit harder than the other, an acceleration begins. This follows the Second Law. When the net force begins going in their direction, the acceleration is in their direction. The movement of the rope slows down until it stops and, if they maintain a higher net force, it begins moving back in their direction.

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    The Third Law is less visible, but it's still present. When you pull on the rope, you can feel that the rope is also pulling on you, trying to move you toward the other end. You plant your feet firmly in the ground, and the ground actually pushes back on you, helping you to resist the pull of the rope. There is an extraordinarily large number of textbooks in theoretical mechanics, because it is a fairly old and well-studied subject.

    You need any textbook on classical mechanics that you can understand and that talks about "Lagrangians" early on. Books that only talk about accelerations, forces, and torques may be quite advanced but they do not cover the subject of theoretical mechanics. From Wikibooks, open books for an open world.

    The latest reviewed version was checked on 25 July Prerequisites The reader should be comfortable with Newton's laws and with basic physics concepts such as mass, moments of inertia, length, force and time q. Suggested books to study There is an extraordinarily large number of textbooks in theoretical mechanics, because it is a fairly old and well-studied subject. Classical mechanics.

    Mechanics | physics |

    An old classic. Hand, J. Analytical mechanics Cambridge,