Keplers Laws and Planetary Movement Essay -- Physics Science Planets

By the turn of the 1600s, the way in which the solar system and the universe as a whole was viewed began to change. With the disputed conclusions of Copernicus, scientists already began to adopt the idea of a heliocentric solar system. Further advancements in astronomy came about through the research of Tycho Brahe and his assistant Johannes Kepler. The three erratic laws developed by Kepler with the data gathered by Brahe shaped the way in which science viewed the structure and motion of the planets of the solar system in sullen ways, lasting to this day.A Brief History of Johannes KeplerJohannes Kepler began his studies in astronomy as an assistant to the astronomer Tycho Brahe, whom, by his own right, was a formidable observer of the heavens, notwithstanding his rather illogical conclusions about the Earth and the movement of other celestial bodies. Brahes observations were phenomenally surgical, especially considering the technology available at the time, often accurate to l ess than half of a minute of arc. In hindsight, however Brahes creditability as an astronomer is diminished due to his lack of acceptance of the idea of a heliocentric solar system created by Copernicus. He agreed that the other five known planets revolved around the sun, but that the Earth would be unable(predicate) of such movement and would certainly be detectable by the inhabitants of the Earth if that were the case.Keplers First LawSince his introduction into astronomy, Kepler had held a strong faith in the accuracy of the theories of Copernicus. Under Copernican theory, all planets traveled in perfectly circular orbits around the sun. However, Keplers observations, especially in regards to the orbit of Mars, suggested that planets trave... ...s Third Law. What else should be celebrated is that the constant (42/Gm) is included in the equation. thus creating an equation that not only proves Keplers Third Law, but is also far reaching in its applicatory applications. For ins tance, if the peroid and distance from the sun of a planet were known, the mass of the planet could easily be calculated.Conclusion The remarkable aspect to Keplers Laws is that they were able to unify the ostensibly complicated motion of the planets in the heavens with relatively simple concepts. The conclusion that the orbits of planets are elliptical rather than circular paved the way into developing elliptical relationships between all the planets by explaining the variance in the velocity of a planet as it travels through its orbit. This proportional relationship, T2 = KR3, merge the motions of the planets beautifully.