Knowledge (XXG)

File:Epicycle and deferent.svg

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il cerchio più piccolo, centrato su un punto del deferente, è l'epiciclo (il suo centro è evidenziato con un punto nero nel disegno, ma ad esso non corrispondeva alcun punto fisico nelle concezioni astronomiche degli antichi); il cerchio rosso pieno è il pianeta, che è centrato su un punto dell'epiciclo; la linea nera spessa rappresenta il moto effettivo del pianeta, che risulta dalla composizione della doppia rivoluzione del deferente intorno alla Terra e dell'epiciclo intorno a un punto del deferente; i punti rossi vuoti rappresentano le successive posizioni del pianeta: visto dalla Terra, esso sembra muoversi in avanti (in direzione est) da 1 a 2, fermarsi in 2, muoversi di moto retrogrado da 2 a 3, fermarsi di nuovo in 3 e poi riprendere il suo moto normale.
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the deferent is the epicycle (its center is highlighted with a black dot in the drawing, but it was no physical body according to ancient astronomers); the filled red dot is the planet, which is centered on a point of the epicycle; the bold black line represents the actual motion of the planet, resulting from the composition of the double revolution of the deferent around the Earth and of the epicycle around a point of the deferent; the empty red dots are consecutive positions of the planet. As seen from the Earth, the planet seems to move forward (eastbound) from 1 to 2, to stop in 2, to move backwards from 2 to 3, to stop again in 3 and then to resume its normal forward motion.
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model as it was used by Apollonius, Hipparcus, Ptolemy and others in order to explain the apparent retrograde motion of planets in a geocentric model. The small circle in the center represents the Earth; the larger circle centered on the Earth is the deferent; the smaller circle centerd on a point of
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qualitativo. Modelli di questo tipo vennero impiegati da Apollionio, Ipparco, Tolomeo e altri per spiegare i moti retrogradi apparenti dei pianeti nei sistemi astronomici geocentrici. Il piccolo cerchio vuoto al centro rappresenta la Terra; il cerchio più ampio, centrato nella Terra, è il deferente;
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This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
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The following pages on the English Knowledge (XXG) use this file (pages on other projects are not listed):
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Corrected eastbound direction as seen from top of the Earth's North Pole
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because it consists entirely of information that is
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Commons is a freely licensed media file repository.
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common property and contains no original authorship
194:), Einaudi, Torino, 2000, p. 78. Also based upon 94: 8: 46:Size of this PNG preview of this SVG file: 719: 486: 377: 311: 604:The following other wikis use this file: 729: 721: 576: 462: 446: 428: 412: 395: 392: 373: 366: 584:Historical models of the Solar System 186:Based upon data from Thomas S. Kuhn, 7: 652:Историски модели на Сончевиот Систем 275:This trigonometry was created with 564:User created page with UploadWizard 475: 712: 386: 380: 292: 274: 253: 156: 143: 126: 76: 385: 371: 335: 286: 268: 247: 93: 31: 21: 368: 157: 144: 14: 367: 26: 1: 36: 393:Items portrayed in this file 688:Usage on tum.wikipedia.org 751: 698:Usage on zh.wikipedia.org 678:Usage on pt.wikipedia.org 658:Usage on nl.wikipedia.org 648:Usage on mk.wikipedia.org 638:Usage on it.wikipedia.org 628:Usage on id.wikipedia.org 618:Usage on as.wikipedia.org 608:Usage on ar.wikipedia.org 188:La rivoluzione copernicana 476: 212: 192:The Copernican Revolution 139:Epicycle and deferent.svg 16: 370: 293:This trigonometry uses 226:Epicycle et deferent.png 196:Epicycle et deferent.png 100:This is a file from the 672:Polemarchus van Cyzicus 642:Utente:MLWatts/Sandbox4 563: 533: 221: 208: 182: 175: 172: 136: 104:. 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File:Epicycle and deferent.svg
560 × 500 pixels
269 × 240 pixels
538 × 480 pixels
860 × 768 pixels
1,147 × 1,024 pixels
2,294 × 2,048 pixels
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Wikimedia Commons
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epicycle-and-deferent
epiciclo-deferente
Epicycle et deferent.png
Julo
MLWatts
Epicycle et deferent.png
Julo

SVG
valid

Inkscape
…important

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