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obliquity of ecliptic - translation to russian
![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.")
[ə'blikwitəs]
прилагательное
общая лексика
имеющий психическое или моральное отклонение
психически или морально извращённый
[ə'blikwiti]
общая лексика
косость
наклон
скос
существительное
общая лексика
отклонение от прямой линии
косое направление
наклонное положение или движение
отклонение от прямого пути
от нормы
(дурная) наклонность
нравственная извращённость
моральное нарушение
туманное
невразумительное высказывание
околичность
нарочитая двусмыслица
двусмысленность (в тексте)
техника
скос
конусность
астрономия
наклонение (орбиты)
наклонение (орбиты)
Definition
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Wikipedia
The ecliptic or ecliptic plane is the orbital plane of Earth around the Sun. From the perspective of an observer on Earth, the Sun's movement around the celestial sphere over the course of a year traces out a path along the ecliptic against the background of stars. The ecliptic is an important reference plane and is the basis of the ecliptic coordinate system.
