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- [[Image:Ecliptic1.png|left|thumb|400px||Fig. 1. The ecliptic is shown as a red circle. Winter and summer refer to the Northern hemispher ...The arrow on the Earth indicates the angle between the Earth axis and the ecliptic plane; it also gives the direction of the diurnal (daily) rotation of the E2 KB (337 words) - 07:00, 10 August 2024
- 102 bytes (14 words) - 11:32, 29 October 2008
- Auto-populated based on [[Special:WhatLinksHere/Ecliptic]]. Needs checking by a human.758 bytes (100 words) - 07:00, 10 August 2024
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- [[Image:Ecliptic1.png|left|thumb|400px||Fig. 1. The ecliptic is shown as a red circle. Winter and summer refer to the Northern hemispher ...The arrow on the Earth indicates the angle between the Earth axis and the ecliptic plane; it also gives the direction of the diurnal (daily) rotation of the E2 KB (337 words) - 07:00, 10 August 2024
- ...another in [[space]]. Conjunctions between two bright objects close to the ecliptic, such as two bright planets, can be seen with the naked eye. When two objects always appear close to the [[ecliptic]]—such as two [[planet]]s, the [[Moon]] and a planet, or the [[Sun]] and1 KB (218 words) - 12:00, 1 August 2024
- ...[Spica]], and [[Regulus]] it is one of the four brightest stars near the [[ecliptic]]. The similarly-colored [[Aldebaran]] (α [[Taurus|Tauri]]) lies almost d538 bytes (74 words) - 07:00, 11 July 2024
- {{r|Ecliptic}}556 bytes (73 words) - 12:52, 22 February 2011
- {{r|Ecliptic}}695 bytes (87 words) - 07:00, 28 July 2024
- {{r|Ecliptic}}718 bytes (91 words) - 17:00, 23 August 2024
- Auto-populated based on [[Special:WhatLinksHere/Ecliptic]]. Needs checking by a human.758 bytes (100 words) - 07:00, 10 August 2024
- {{r|Ecliptic}}910 bytes (118 words) - 12:00, 10 September 2024
- {{r|Ecliptic}}1 KB (142 words) - 12:01, 19 September 2024
- ...these trans-Neptunian bodies orbit the Sun within a thick band around the ecliptic plane of the solar system. For this reason it is largely believed that they Pluto has an eccentric orbit: it is inclined 17 degrees to the ecliptic plane and ranges from 29.7 AU from the Sun at perihelion (within the orbit3 KB (560 words) - 07:00, 9 September 2024
- ...een successive vernal equinoxes. The mean tropical year (averaged over all ecliptic points) is 365.242 189 67 days (365d 5h 48min 45s) long.6 KB (968 words) - 01:12, 14 February 2010
- ...simply converted Hipparchus's description of the location of each star to ecliptic coordinates and then shifted these values by a constant to account for prec4 KB (622 words) - 07:00, 9 July 2024
- {{r|Ecliptic}}2 KB (303 words) - 20:42, 11 January 2010
- {{r|Ecliptic}}2 KB (308 words) - 10:38, 25 June 2024
- ...een successive vernal equinoxes. The mean tropical year (averaged over all ecliptic points) is 365.242 189 67 days (365d 5h 48min 45s) long.7 KB (1,171 words) - 00:02, 14 February 2010
- ...rial plane makes an angle of 23° 26' with the ecliptic. See the article [[ecliptic]] for illustrations.5 KB (857 words) - 10:54, 22 March 2010
- In addition, for the Chinese, the region of sky passed through by the [[ecliptic]] is not divided into 12 [[zodiac|zodiacal constellations]], but into '''Tw5 KB (655 words) - 07:00, 28 July 2024
- ...of the planet tilted just over 90 degrees with respect to the poles of the ecliptic (the plane of the planet's revolution about the Sun). Thus the rotational a7 KB (1,187 words) - 04:17, 14 September 2024
- ...eriod of 18.61 years during Earth's orbit around the Sun. The plane of the ecliptic in turn is itself about 23 degrees from the plane of the Earth's equator.<r18 KB (2,981 words) - 07:01, 21 September 2024
- ...apparent motion of the Sun as seen from Earth; it introduces concepts as [[ecliptic]], winter/summer [[solstice]] and vernal/autumnal [[equinox]]. When the a ...ual orbit, whereas in reality it makes a constant angle with the invariant ecliptic. Therefore, Copernicus had to introduce an extra conical yearly motion to23 KB (3,632 words) - 18:47, 8 April 2014