ecliptic hurpeh Fr.: écliptique The Sun’s apparent path in the sky relative to the stars in the course of a year. It is also the projection of the Earth’s orbital plane onto the → celestial sphere. Because of the inclination of the → Earth’s rotation axis, the ecliptic is tilted by about 23.4° with respect to the → celestial equator, an angle known as the → obliquity of the ecliptic. The ecliptic crosses the celestial equator at the → equinoxes. Etymology (EN): From L. ecliptica linea “path of eclipses,” so called because eclipses
happen only when the Moon is near this path, from eclipsis, Etymology (PE): Hurpeh “sun path,” from hur “sun,” variant xor, cognate with Gk.
helios, → Sun, +
peh “path, way,” from O.Pers. paθi- “path, way;”
Av. paθ-, variants paθi-, paθā-, pantay-; |