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The Scientific Revolution

Nicolaus Copernicus (1473 1543) was obviously a Renaissance polymath responsible for what many have called the “Copernican Revolution”. Among Copernicus’ most crucial contributions was the field of astronomy. Copernicus placed the sun in the middle of the universe, instead of planet Earth. The earlier system, the Ptolemaic model, was geocentric (with the Earth in the middle of the universe). In 1543, in his “On the Revolutions of the Celestial Spheres”, he published his theory (which he had developed much earlier). While he still had the planets going in patterns of circles rather than ellipses, he postulated that these circles had no ease. Although it is the center of gravity and the lunar sphere, he said that the middle of the Earth is not the center of the universe. He mentioned that the Earth is one of the 7 planets of the solar system in the Sun, that is, stationary. He stated that the rotation of the Earth is included in the movements, the revolution and the annual tilt of the axis. He agreed with experts before him that the distance from Earth to sunlight is negligible compared to the distance from Earth to stars. Tycho Brahe was among the successors of Copernicus; however, the Tychonic system was essentially a geocentric model comprising several mathematical underpinnings of heliocentric versions.

Galileo Galilei (1564-1642) designed on the basis of the career of Copernicus. Additionally, a strong proponent of heliocentric design, Galileo was placed under house arrest for much of his life for his beliefs after being tried in Rome. He was known as a heretic for thinking that the Sun, not the Earth, was the motionless center of the universe. In recent years, the Church has recognized that its control of the Galileo affair was regrettable. In 1610, Galileo printed “The Starry Messenger”, which reported the discoveries of his four moons of Jupiter, the roughness of the Moon’s surface, the stars invisible to the naked eye, and the differences between the appearances of the planets in addition fixed stars. . He further published observations on the full range of Venus phases and published on tides. Galileo’s theory was that the tides were caused by the ebb and flow of water in the seas at one location on the Earth’s surface which accelerated at certain times of the day due to the rotation of Earth. However, this is incorrect (because the tides are caused by the moon). Galileo also put forward the fundamental idea of ​​relativity (the rules of physics are exactly the same in any system that moves at frequent speed in a straight line). Galileo was among the first to observe a sunspot without erroneously attributing it to a transit of Mercury. Galileo also showed that falling bodies of similar materials but different masses have identical descent times. Essentially, the fall time is mass-free. Galileo also demonstrated that there are as many perfect squares as there are whole numbers, although most numbers are not ideal squares; since you will find non-squares and squares, and only a few digits are squares, there should be fewer squares than non-square numbers. However, for every number there is a square. So there is actually a 1:1 ratio of non-squares to squares.

Johannes Kepler (1571-1630) is responsible for producing Kepler’s regulations of planetary motion. These laws include that the orbit of each Earth is an ellipse with the Sun among the two foci, that a line connecting the Sun and a planet sweeps out equal parts for equal times, that the square of the orbital time of any planet is specifically proportional to the cube of a semi-major axis of its orbit. Kepler was among the first to add the field of physics as well as the field of astronomy. This sparked some controversy, but his concepts gained much more reading and acceptance after his death. Once Newton derived Kepler’s laws from a common gravitational principle, they became part of the theoretical canon of the Scientific Revolution.

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