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Johannes Kepler Research Paper

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This paper will discuss the life of the German mathematician, astronomer, and astrologer Johannes Kepler. Who had a great impact in the 17th century scientific revolution, because of his development of the three laws of planetary motion. He is also remembered for the legacy he left that later provided one of the foundations for Isaac Newton's theory of universal gravitation.
“Johannes Kepler was born on December 27, the feast day of St John the Evangelist, 1571, in the Free Imperial City of Weil der Stadt (now part of the Stuttgart Region in the German state of Baden-Württemberg”. The is not a lot of information about his parents. Its alleged that his father left when he was five and never returned, possibly killed in war. While her mother …show more content…

Later, this was the base of what it’s now the laws of gravity, which Isaac Newton placed together after more or less 30 years after the death of Kepler.
Around the beginning of 1600, Kepler presented three laws of planetary motion. He was capable of recollecting all the work of his mentor Tycho Brache, and summarized to three main laws that explained the motion of planets in a sun-centered solar system. Later with more research and experiments, it was discovered that all Kepler's work about this laws weren’t exactly truth. Nonetheless, this laws are still considerate respectable descriptions of the motion of any planet and any satellite.
First law, known as the law of ellipses, establishes that the planets are revolving or orbiting the sun in a path identified as an ellipse. “An ellipse is a special curve in which the sum of the distances from every point on the curve to two other points is a constant. The two other points are known as the foci of the ellipse”. The shorter the distance between these points is, the more similar is the ellipse to the shape of a circle. As a matter of fact, when these points are at the same location, they are the special case of an ellipse known as a circle. “Kepler's first law is rather simple - all planets orbit the sun in a path that resembles an ellipse, with the sun being located at one of the foci of that ellipse” (The Physics

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After Brache’s death, Kepler inherited his astronomical data. Johannes Kepler of Germany was inspired by the Neoplatonism and his continues sighting of Brahe, he set forth his solution for what is keeping the planets in their orbits. Kepler was able to affirm that the solar system itself is regular and it is organized by mathematically determined relationships. Both Tycho Brahe of Denmark and Johannes Kepler of Germany laid groundwork for Isaac Newton and his

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This goes hand in hand with Newton's Laws of motion and universal gravitation. Newton's law of universal gravitation states that a particle attracts every other particle in the universe using a gravitational force and Newton's law of motion states that every object will remain at rest or in uniform motion in a straight line unless compelled to change its state by the action of an external force. Newton's Laws back up Kepler's laws by explaining how the planets orbit is an ellipse with the Sun at one of the two foci or center. The force that allows this to happen to the planets are explained by Newton's law and that the gravitational force is moving the planets into rotation, as by the law of motion. These forces assisting each other can make phenomenon's occur such as tides.

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1. Describe the three laws of planetary movement formulated by Johannes Kepler. -The law of Ellipse: This is the first law of John Kepler which states that planets circulate around the sun in in ellipse, with the sun on one focus (Stern: 2014). The law of equal areas:

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The most important piece of information is that he created the three major laws of planetary motions. His first law explains that the planets orbit the Sun in a route describe as an ellipse. The second law states the speed of any given planet while it orbits the sun. The third and final law

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Johannes Kepler was a German astronomer, mathematician and theologist. Kepler was born in Weil der Stadt, near to Stuttgart, in 1571. Johannes Kepler is nowadays most famous for developing the three laws of planetary motion in the early 17th century. Johannes Kepler’s family was a very poor family, his father left him when he was only five, and because he was prematurely born, he was a very weak child and was ill a lot. These were not optimal circumstances for someone, who made it very far in his later life and resisted all of the negative conditions.

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The Tycho Brahe's contributions to Kepler’s Laws of Planetary Motion In the book, “figure 2.12, Tycho Brahe in his observatory Uraniborg, on the island of Haven in Denmark. Brahe’s observations of the positions of stars and planets in the sky were the most accurate and complete set of naked eye measurements ever made. When the Tycho moved to Prague, as the Imperial mathematician of the Holy Roman Empire happens to be fairly close to Graz, in Austria, the Kepler lived and worked. Kepler joined Tycho in Prague in 1600 and put to work trying to find a theory that could explain Brahe’s planetary data.

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Because the sun us much heavier than any planet, Keplers third law correlates to Newtons equations (Laws Of Planetary Motion,

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During the Middle Ages a Roman Astronomer named Ptolemy came up with the theory that all surrounding planets orbited around the Earth. Advancement in telescopes and technology helped Copernicus during the renaissance create a more logical and accurate theory which stated how the sun is in the middle of our universe and all planets orbited the sun. This changed the way man thought because it realized how small Earth is compared to the rest of the solar system and how we may not be

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He realized that a planet moved slower farther away from the sun than it did when closer. Once he understood that planets traveled in ellipses, he determined that a line connecting the sun to a planet covered an equal amount of area over the same amount of time. This is Kepler’s Second Law. Kepler's Third Law was published a decade later, and recognized the relationship between the periods of two planets and their distance from the sun.

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