Johannes Kepler Research Paper

Improved Essays
Kepler’s Laws, Kepler is credited with 3 laws regarding the movement of celestial bodies orbiting other celestial bodies. Johannes Kepler, working with data painstakingly collected by Tycho Brahe without the aid of a telescope, developed three laws which described the motion of the planets across the sky. Kepler's 1st Law: The Law of Orbits, Kepler's 2nd Law: The Law of Areas, and Kepler’s 3rd Law: The Law of Periods. Kepler's laws were derived for orbits around the sun, but they apply to satellite orbits as well. In retrospect, the reason that the orbit of Mars was particularly difficult was that Copernicus had correctly placed the Sun at the center of the Solar System, but had erred in assuming the orbits of the planets to be circles. Thus, in the Copernican theory epicycles were still required to explain the details of planetary motion.
It fell to Kepler to provide the final piece of the puzzle: after a long struggle, in which he tried mightily to avoid his eventual conclusion, Kepler was forced finally to the realization that the orbits of the planets were not the circles demanded by Aristotle and assumed implicitly by Copernicus, but were instead the "flattened circles"
…show more content…
For simplicity, we'll consider the motion of the planets in our solar system around the Sun, with gravity as the central force. Among other things, Kepler's laws allow one to predict the position and velocity of the planets at any given time, the time for a satellite to collapse into the surface of a planet, and the period of a planet's orbit as a function of its orbits' geometry. Though the laws were originally obtained by Kepler after careful analysis of empirical data, the complete understanding was missing until Newton derived each law as pieces of his orbital mechanics. In his footsteps we will obtain each law in turn, as we consider the orbit of a planet in the gravity of a massive

Related Documents

  • Improved Essays

    Copernicus died in May, one year later. Nicolaus Copernicus was an extremely successful scientist and astronomer who lived during the Renaissance. During this time period it was a common to believe that the Earth was at the center of the universe. It wasn’t until Copernicus proposed the heliocentric theory. This theory that he had made declared that the planets revolve around the sun, and…

    • 162 Words
    • 1 Pages
    Improved Essays
  • Improved Essays

    Long ago, people believed that the Earth was the center of the universe, and that all the stars, planets, and other celestial bodies orbited around it. However, as pivotal discoveries were made and new theories emerged, society gained a much more insightful understanding of the cosmos above. In the second century, an astronomer by the name of Claudius Ptolemy proposed his geocentric model of the solar system, which depicted Earth in the center of the universe and the planets and the Sun orbiting in concentric circles around it. There were problems with this model, however, and years later an astronomer named Nicolaus Copernicus proposed another model which showed the Sun at the center.…

    • 799 Words
    • 4 Pages
    Improved Essays
  • Decent Essays

    Both of these men believed that their theories about the planets were accurate. You had Copernicus who believed that all planets orbited the sun while the moon orbited the earth. He was also convinced that the sun was in the center and did not move, and neither did the stars. As for Ptolemy, he believed that all objects orbited the sun. His theory was that the Earth was the center of the universe but stayed still.…

    • 76 Words
    • 1 Pages
    Decent Essays
  • Improved Essays

    Lbo Research Paper

    • 482 Words
    • 2 Pages

    The objects between 42 and 47 AU are in very stable orbits – not affected in any significant way by any of the planets. Like the “classical” planets, these objects are in nearly circular orbits, so were given the name “Classical KBOs” (CKBOs), by David Jewitt. Of the CKBOs, about one-third have a low orbital inclination of around 2o – these are the “Cold” CKBOs. The remaining two-thirds have a much higher inclination of up to 20o or more – the “Hot” CKBOs. Hot and cold do not have anything to do with temperature here – hot refers to highly inclined orbits.…

    • 482 Words
    • 2 Pages
    Improved Essays
  • Improved Essays

    What was the motivation that led to the discovery? William Herschel was an accomplished musician in 18th century England. After achieving musical success his interests turned to the stars. He and his sister Caroline began cataloguing stars, keeping track of their positions, movements and taking many notes. Caroline is credited with keeping the notes organized and up to date.…

    • 323 Words
    • 2 Pages
    Improved Essays
  • Improved Essays

    Johannes Kepler had an unique life which had many peaks and many valleys, he was born December 27,1571. His childhood was very rough because his parents were very poor and he was a sickly child. Their family had no money for medicine and his illness. Fortunately his intelligence bought him a scholarship to a very nice college.…

    • 569 Words
    • 3 Pages
    Improved Essays
  • Improved Essays

    In the beginnings of the creation of a model of our planetary system, Greek philosopher Aristotle stated that Earth could be found at the center of the universe, giving birth to an idea called "geocentrism" around 300 B.C. This belief consisted of planets orbiting Earth in perfectly circular paths called "epicycles". This worked for a while, but as more and more observations were done, the model started to fall apart, with a multitude of additional corrections changing the model until it was no longer thought to be valid. It should be worth noting that around the same time but a little later, a Greek astronomer named Aristarchus of Samos constructed a model which proposed all the planets revolved around the Sun, however, because Aristotle had a much stronger influence, Aristarchus' ideas didn't catch on until after his death. This is when Claudius Ptolemaeus started to introduce his updated model around 140 A.D.…

    • 762 Words
    • 4 Pages
    Improved Essays
  • Decent Essays

    There, he studied to become a lutheran minister and the work of Nicolaus Copernicus in 1589. His accomplishments impacted many people the way we see space now. One of Kepler’s famous discoveries included the three major laws of planetary motion. He found a solution to fix farsighted and nearsighted-ness by creating glasses.…

    • 151 Words
    • 1 Pages
    Decent Essays
  • Improved Essays

    leaving the shore to effectively illustrate this point, he writes, “...when a ship floats on over a tranquil sea, all the things outside seem to the voyagers to be moving in a movement which is the image of their own” (13). This optical illusion mirrors the geocentrism Copernicus was attempting to dispel. Copernicus also noted that clouds and falling objects are not affected by the rotation of the Earth because they obey the same nature as earth. 9. “Whether Many Movements can be Attributed to The Earth, and Concerning the Center of the World.”…

    • 1194 Words
    • 5 Pages
    Improved Essays
  • Improved Essays

    Newton’s improvement of Galileo’s law of gravitational force is denoted the title of…

    • 1241 Words
    • 5 Pages
    Improved Essays
  • Improved Essays

    Dark Matter Research Paper

    • 1042 Words
    • 5 Pages

    The formula to give the orbital velocity for a satellite is: V=√(GM/r) (Blackman, n.d.) While the Law of Universal Gravitation…

    • 1042 Words
    • 5 Pages
    Improved Essays
  • Improved Essays

    (Wikipedia, Astronomia Nova, n.d.) His first laws stated that all planets move around the Sun in an elliptical orbit, having the Sun at one of the two foci, also sometimes referred to as the law of ellipses. We can use the formula r=p/(1+ecosx) to represent an ellipse. where P is the semi-latus rectum, and ε is the eccentricity of the ellipse, and r is the distance from the Sun to the planet, and θ is the angle to the planet's current position from its closest approach, as seen from the Sun. Kepler’s second law states That the speed of the planet changes at each moment such that the time between two positions is always proportional to the area swept out on the orbit between these positions (Wikipedia, Kepler's laws of planetary motion, n.d.).…

    • 677 Words
    • 3 Pages
    Improved Essays
  • Improved Essays

    After these values are obtained and changed into the proper unit of distance and time, meters and seconds, they can be plugged into Kepler’s Third Law: The first step to calculating the equation is to take the first half and multiple across. Meaning obtain pi and then square its value and multiply it by four.…

    • 701 Words
    • 3 Pages
    Improved Essays
  • Great Essays

    Newton’s law of gravity states that every object fall to the ground at the same speed. Even though Galileo had accomplished many things for science, “Galileo believed that his most important scientific contribution was his application of mathematics to the study of motion…” (Whitehouse 216). Galileo made many things possible for future scientists and astronomers. But many scientists and astronomers before Galileo made it possible for him as well.…

    • 1637 Words
    • 7 Pages
    Great Essays
  • Improved Essays

    This demonstrates the accuracy and validity of mathematics, even though it is impossible for Newton to witness, observe or sense the forces in the solar system, he managed to discover the elliptical orbit trend. Moreover, Newton used his sense experience when he saw an apple falling down from a tree, meaning the apple has a downward acceleration. He concluded that this downward motion of an object is associated to the mass of (“Newton's Law of Universal Gravitation.”), thus created a mathematical equation for his second law. Mathematical formulas help increasing the objectivity of his idea on the principle as it hides the subjectivity of sense perceptions. So, creating a shared knowledge which is recognized by the global…

    • 789 Words
    • 4 Pages
    Improved Essays