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WOU ES 104 - Birth of Modern Astronomy Celestial Motion

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1Lab starts this week—NS 017Bring lab manual to labBring lab manual to labDo Prelab 1 before you go! Ancient civilizations believed that Earth was at the center of the universe—GEOCENTRIC MODEL Age of Reason beginning to recognize Sun is center of Solar System—HELIOCENTRIC MODEL Age of Technology exploring wide reaches of the universe 5thcentury B.C. Moon is a sphere lighted by Sun•http://www-history.mcs.st-andrews.ac.uk/Biographies/Anaxagoras.html 4thcentury BC Earth is a sphere•http://www.hao.ucar.edu/public/education/sp/images/aristotle.html 3rdcentury BC Mathemetician Placed Sun at center with Earth orbiting itwith Earth orbiting it•http://en.wikipedia.org/wiki/Eratosthenes#Measurement_of_the_Earth 2ndcentury AD Copies of works survive to this dayTltd t Translated to Arabic early, to Latin in 13thcentury•http://archive.ncsa.uiuc.edu/SDG/Experimental/vatican.exhibit/exhibit/full-images/d-mathematics/math21.gif Mars usually moves across sky west to east Occasionally appears to move east to west Occurs when Earth is ‘passing’ Mars2 Thought Earth was the unmoving center Translated into Latin in 13thcentury Influenced intellectual thought for centuries Earth would fly apart if it rotated on an axis Moon would be left behind if Earth orbited Sun Since God created Earth and Sun and all the heavenly bodies, Earth is the center of the heavenly bodies, Earth is the center of the universe Earth rotates on an axis, instead of everything orbiting Earth Earth orbits Sun like the planets, so it a planet too “On the Revolution of the Heavenly Spheres”, 1543http://www.hao.ucar.edu/public/education/sp/images/copernicus.html Detailed observations of movement of planetshttp://www.hao.ucar.edu/public/education/sp/images/tycho.html His careful observations and records are his most important legacyhttp://www.hao.ucar.edu/public/education/sp/images/tycho.3.htmlhttp://www.hao.ucar.edu/public/education/sp/images/tycho.1.html http://www.hao.ucar.edu/public/education/sp/images/tycho.2.html3 Discounted Copernicus model because he could not discern stellar parallax It does exist, he didn’t have tools to see ithttp://www.hao.ucar.edu/public/education/sp/images/tycho.4.html Tycho’s assistant and successor Used Tycho’s data to determine planetary determine planetary orbits are ellipticalhttp://en.wikipedia.org/wiki/Image:Johannes_Kepler.jpg Orbit of planet is ellipse Sun at one Focus Equal areas in equal time intervals accounts for the uneven speeds p2=d3p=Period (time to orbit Sun) in Earth yearsd=Distance in Astronomical Units: 1 A.U.=distance from Earth to Sun Strong supporter of Copernican model of planetary movement Built 30x telescopes u lt 30 telescopes (from descriptions of the devices) and looked at planets and Moon starting in 1609http://en.wikipedia.org/wiki/Galileo_Galilei#Technology Telescope used to see that another body in solar system is a center of orbital movement These moons are not left behind, and Earth’s Moon is not either4 When viewed by telescope, planets look like discs, not points of light as stars do Jupiter has moonsVenus has phasesVenus has phases Moon’s surface has texture Sun rotates on an axis Explained the orbital motion of planets as the interaction of inertia and gravity Invented the calculus to simplify his calculations of motion Sun is at the center of the solar system Published by Copernicus Supported by Galileo’s telescopic observations of Jupiter and Venus Kepler determined orbits are ellipses Newton determined orbits created by interaction of inertia and gravity 1851 Supports that Earth does rotate on its axis—Copernicus’


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WOU ES 104 - Birth of Modern Astronomy Celestial Motion

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