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・ Oenomaus nigra
・ Oenomaus of Gadara
・ Oenomaus ortygnus
・ Oenomaus poirieri
・ Oenomaus taua
・ Oenomel
・ Oenomys
・ Oenone
・ Oenone (disambiguation)
・ Oenone (poem)
・ Oenone Wood
・ Oenonella
・ Oenophilia
・ Oenopia
・ Oenopia conglobata
Oenopides
・ Oenopides (crater)
・ Oenopion
・ Oenopota
・ Oenopota admetoides
・ Oenopota alba
・ Oenopota bicarinata
・ Oenopota biconica
・ Oenopota blaneyi
・ Oenopota cancellata
・ Oenopota candida
・ Oenopota casentina
・ Oenopota cinerea
・ Oenopota cingulata
・ Oenopota convexigyra


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Oenopides : ウィキペディア英語版
Oenopides
:''For the lunar crater, see Oenopides (crater)''.
Oenopides of Chios ((ギリシア語:Οἰνοπίδης)) was an ancient Greek mathematician (geometer) and astronomer, who lived around 450 BCE. He was born shortly after 500 BCE on the island of Chios, but mostly worked in Athens.
== Astronomy ==
The main accomplishment of Oenopides as an astronomer was his determination of the angle between the plane of the celestial equator, and the zodiac (the yearly path of the sun in the sky). He found this angle to be 24°. In effect this amounted to measuring the inclination of the earth axis. Oenopides's result remained the standard value for two centuries, until Eratosthenes measured it with greater precision.
Oenopides also determined the value of the Great Year, that is, the shortest interval of time that is equal to both an integer number of years and an integer number of months. As the relative positions of the sun and moon repeat themselves after each Great Year, this offers a means to predict solar and lunar eclipses. In actual practice this is only approximately true, because the ratio of the length of the year and that of the month does not exactly match any simple mathematical fraction, and because in addition the lunar orbit varies continuously.
Oenopides put the Great Year at 59 years, corresponding to 730 months. This was a good approximation, but not a perfect one, since 59 (sidereal) years are equal to 21550.1 days, while 730 (synodical) months equal 21557.3 days. The difference therefore amounts to seven days. In addition there are the interfering variations in the lunar orbit. However, a 59-year period had the advantage that it corresponded quite closely to an integer number of orbital revolutions of several planets around the sun, which meant that their relative positions also repeated each Great Year cycle. Before Oenopides a Great Year of eight solar years was in use (= 99 months). Shortly after Oenopides, in 432 BC, Meton and Euctemon discovered the better value of 18 years, equal to 223 months (the so-called Saros period).

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