Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

Ptolemy and Copernicus: Ancient and Modern Cosmological Models - Prof. Elizabeth Anne Lada, Study notes of Astronomy

An overview of the geocentric model of the universe developed by ptolemy in the 1st century ad and the heliocentric model proposed by copernicus in the 16th century. The key features of each model, including the use of eccentrics, epicycles, and the equant in ptolemy's model, and the assumptions of uniform, circular motions and the placement of the sun at the center of the cosmos in copernicus' model. The document also touches upon the influence of aristotle, plato, and pythagoras on these astronomers' work.

Typology: Study notes

Pre 2010

Uploaded on 03/18/2009

koofers-user-tjs-1
koofers-user-tjs-1 🇺🇸

10 documents

1 / 5

Toggle sidebar

Related documents


Partial preview of the text

Download Ptolemy and Copernicus: Ancient and Modern Cosmological Models - Prof. Elizabeth Anne Lada and more Study notes Astronomy in PDF only on Docsity! 1 Ptolemy (125 A.D.) • Designed a complete geometrical model of the universe that accurately predicted planetary motions with errors within 50 • Most of the geometric devices and basic foundations of his model did not originate with him but were based on the models of the early Greeks such as Aristotle & Hipparchus • Wrote the Almagest (Greatest) – included the original works & models of Ptolemy – included a compilation of past works of Greeks, especially Hipparchus – 13 volumes Ptolemy’s Model • Earth was spherical & at center of cosmos - GEOCENTRIC • Cosmos is finite in size • Earth has no motions • Sun, Moon Planets exhibit uniform, circular motions – natural motions - no forces • Used devices of eccentrics, epicycles & deferents to explain the observed non-uniform motions of the Sun and planets along the ecliptic & retrograde motion. • Introduced equant to explain the variations in retrograde motions Ptolemy’s Equant • point inside a circle, not at the center, from which motion along the circumference of the circle would appear to be uniform • opposite the circle’s center from the eccentric (the Earth) • nonphysical geometrical device that broke fundamental assumption of uniform circular motion Celestial motions no longer had to be uniform around the centers of circles Ptolemy’s Model Copernicus (1473-1543) • Developed a Heliocentric (Sun centered) model of the cosmos • Why? Ptolemy’s geocentric model lasted for centuries mainly because it accurately predicted celestial motions so there was little reason to discard it • Copernicus studied the works of Aristotle, Pythagoras & Plato • an offshoot of Plato’s philosophy asserted that Sun was godhead of all knowledge • Copernicus objected to equant based on aesthetics - equant not faithful to ideal of uniform motion - makes models to complex Copernicus’ Model • Copernicus worked on his new Heliocentric model for 20 years – Sun was placed at center of cosmos – Earth no longer static, but revolved around Sun once a year & rotated on axis once a day • His work was published in De revolutionibus in the year of his death • De revolutionibus took after the Almagest in outline and basic intention - to explain planetary motions • Even though it took 20 years to develop this model did predict celestial motions any better than Ptolemy’s geocentric model 2 Heliocentric Model of Copernicus • Cosmos finite in size • Assumed no forces for heavenly motions – Physics of Aristotle • Assumed uniform, circular motions – done for aesthetics - followed Aristotle • All heavenly spheres revolve around the sun & the sun is at the center of the cosmos – chosen based on aesthetics and simplicity • The distance from the earth to the sphere of stars is much greater than the distance from the earth to the sun – accounts for lack of observed stellar parallax Heliocentric Model of Copernicus • The daily motion of the heavens relative to the horizon results from the earth’s motion on its axis – aesthetic appeal since only 1 sphere is rotating not many – however, he did not account for the objection that if the earth rotated, objects should be flung from the surface • The apparent motion of the sun relative to the stars results from the annual revolution of the earth around the sun • The planets’ retrograde motion occur from the motion of the earth relative to the other planets – retrograde explained as a natural result of the planet’s revolutions about sun - what we observe is an illusion Retrograde Motion Explained Retrograde Motion Explained • When the earth passes any of the outer planets or when the earth is passed by the inner ones, retrograde motion occurs • Passing is key to retrograde motion in the heliocentric model • Copernicus eliminated epicycles to explain retrograde motion • Eliminated equant - kept uniform circular motion • Needed to account for variations in planetary motion so he was forced to add many smaller circles • Violated Aristotelian physics & did not offer new physical ideas to support his model • Didn’t predict motions any better than Ptolemy’s model Copernican Model Ptolemy
Docsity logo



Copyright © 2024 Ladybird Srl - Via Leonardo da Vinci 16, 10126, Torino, Italy - VAT 10816460017 - All rights reserved