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эклиптический - translation to English
эклиптический
adj.
ecliptic
ecliptic
ecliptic coordinates
![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.")
![z}}-axis points toward the north [[ecliptic pole]]. The reference frame is relatively stationary, aligned with the vernal equinox.](https://commons.wikimedia.org/wiki/Special:FilePath/Heliocentric rectangular ecliptic.png?width=200 "z}}-axis points toward the north [[ecliptic pole]]. The reference frame is relatively stationary, aligned with the vernal equinox.")
CELESTIAL COORDINATE SYSTEM USED FOR REPRESENTING THE POSITIONS OF SOLAR SYSTEM OBJECTS
Ecliptic coordinates; Ecliptic longitude; Ecliptic latitude; Mean equinox
математика
эклиптические координаты
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.")
APPARENT PATH OF THE SUN ON THE CELESTIAL SPHERE
Plane of the ecliptic; Astronomical ecliptic; Ecliptic circle; Ecliptic plane; Plane of ecliptic; Eclyptic
[i'kliptik]
прилагательное
общая лексика
потускневший
потерявший блеск
астрономия
эклиптический
существительное
[i'kliptik]
астрономия
эклиптика
Definition
эклиптический
прил.
1) Соотносящийся по знач. с сущ.: эклиптика, связанный с ним.
2) Свойственный эклиптике, характерный для нее.
1) Соотносящийся по знач. с сущ.: эклиптика, связанный с ним.
2) Свойственный эклиптике, характерный для нее.
