The Obliquity of the Ecliptic Pytheas Measures

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The Obliquity of the Ecliptic Pytheas Measures

PYTHEAS MEASURES LOCATING THE OBLIQUITY OF THE ECLIPTIC Pytheas of Marseille (about 300 BC), sailor and astronomer. He made a famous trip to the limits of Northern Europe and made several astronomical measurements. The obliquity of the ecliptic is the angle between the Earth's orbital plane and the plane of the Earth's axis of rotation Evocation of Marseille at the time of Pytheas © J-M.Gassend equator. This angle allows astronomers to detect the obliquity movement of stars and planets in the sky. plane of equator What is the process of Pytheas ? summer solstice ecliptic plane of orbit equinox obliquity gnomon horizontal plane Pytheas uses a gnomon (vertical obelisk) measuring its shadow at the South North summer solstice and then at the equinox. The angle between the two radii is the looked-for angle. shadows of gnomon How Pytheas calculated the angle ? The vertical figure is first transferred to the ground in order to make the measurements more easy. The angle is measured as a fraction of total circumference, which was equinox shadow common at the time. solstice shadow South North The angle can be put 15 times in the circumference and there is a remainder. This remainder can be put 11 times in the angle, we neglect the second rest appearing. The circumference contains 15x11 + 1 = 166 times the rest, the angle is thus 11/166, which is 23°51', slightly higher than the current value 23°27' because of the long-term variations of the inclination of the axis of the Earth. 11 1 The writing = 1 11 166 15 + 10 11 9 is what is named now a 8 continued fraction 7 6 5 4 3 2 1 IREM Aix-Marseille http://www.irem.univ-mrs.fr/expo2013.

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