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эклиптика - translation to English
![publisher=[[Астронет]]}}</ref>](https://commons.wikimedia.org/wiki/Special:FilePath/Plane of Ecliptic.jpg?width=200 "publisher=[[Астронет]]}}</ref>")
ecliptic
![polar axis]] (green). The plane of the ecliptic intersects the celestial sphere along a [[great circle]] (black), the same circle on which the Sun seems to move as Earth orbits it. The intersections of the ecliptic and the equator on the celestial sphere are the vernal and autumnal [[equinox]]es (red), where the Sun seems to cross the celestial equator.](https://commons.wikimedia.org/wiki/Special:FilePath/Earths orbit and ecliptic.PNG?width=200 "polar axis]] (green). The plane of the ecliptic intersects the celestial sphere along a [[great circle]] (black), the same circle on which the Sun seems to move as Earth orbits it. The intersections of the ecliptic and the equator on the celestial sphere are the vernal and autumnal [[equinox]]es (red), where the Sun seems to cross the celestial equator.")
![tilted]] five degrees to the ecliptic) results in the revolution of the [[lunar nodes]] relative to the Earth. This causes an [[eclipse season]] approximately every six months, in which a [[solar eclipse]] can occur at the [[new moon]] phase and a [[lunar eclipse]] can occur at the [[full moon]] phase.](https://commons.wikimedia.org/wiki/Special:FilePath/Eclipse vs new or full moons, annotated.svg?width=200 "tilted]] five degrees to the ecliptic) results in the revolution of the [[lunar nodes]] relative to the Earth. This causes an [[eclipse season]] approximately every six months, in which a [[solar eclipse]] can occur at the [[new moon]] phase and a [[lunar eclipse]] can occur at the [[full moon]] phase.")
![url = https://books.google.com/books?id=WTEaAAAAYAAJ&q=dziobek+mathematical}}, p. 294, at Google books</ref> This is the inclination to the ecliptic of 101,800 CE. Note that the ecliptic rotates by only about 7° during this time, whereas the [[celestial equator]] makes several complete cycles around the ecliptic. The ecliptic is a relatively stable reference compared to the celestial equator.](https://commons.wikimedia.org/wiki/Special:FilePath/Ecliptic inclination dziobek.PNG?width=200 "url = https://books.google.com/books?id=WTEaAAAAYAAJ&q=dziobek+mathematical}}, p. 294, at Google books</ref> This is the inclination to the ecliptic of 101,800 CE. Note that the ecliptic rotates by only about 7° during this time, whereas the [[celestial equator]] makes several complete cycles around the ecliptic. The ecliptic is a relatively stable reference compared to the celestial equator.")
![equatorial coordinates]] (blue), being inclined to the ecliptic, appear to wobble as the Sun advances.](https://commons.wikimedia.org/wiki/Special:FilePath/Ecliptic vs equator small.gif?width=200 "equatorial coordinates]] (blue), being inclined to the ecliptic, appear to wobble as the Sun advances.")
Definition
Wikipedia
Экли́птика (от лат. (linea) ecliptica, от др.-греч. ἔκλειψις — затмение) — большой круг небесной сферы, по которому происходит видимое с Земли годичное движение Солнца относительно звёзд. Соответственно, плоскость эклиптики — это плоскость обращения Земли вокруг Солнца (плоскость земной орбиты). Современное, более точное определение эклиптики — сечение небесной сферы плоскостью орбиты обращения вокруг Солнца барицентра системы Земля — Луна.
Все известные планеты Солнечной системы и большинство других тел в ней движутся вблизи плоскости эклиптики в том же направлении, что и Земля. Созвездия, лежащие в плоскости эклиптики, называются зодиакальными созвездиями. Плоскость эклиптики является фундаментальной плоскостью эклиптической системы координат, в которой координаты светила выражаются эклиптической широтой и эклиптической долготой.
