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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 (333 words) - 05:31, 24 March 2010
- 12 bytes (1 word) - 11:31, 29 October 2008
- | pagename = Ecliptic | abc = Ecliptic2 KB (224 words) - 07:19, 15 March 2024
- 102 bytes (14 words) - 11:32, 29 October 2008
- Auto-populated based on [[Special:WhatLinksHere/Ecliptic]]. Needs checking by a human.579 bytes (76 words) - 16:10, 11 January 2010
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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 (333 words) - 05:31, 24 March 2010
- ...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 (214 words) - 13:01, 18 November 2022
- | pagename = Ecliptic | abc = Ecliptic2 KB (224 words) - 07:19, 15 March 2024
- ...[Spica]], and [[Regulus]] it is one of the four brightest stars near the [[ecliptic]]. The similarly-colored [[Aldebaran]] (α [[Taurus|Tauri]]) lies almost d507 bytes (70 words) - 16:41, 30 December 2008
- {{r|Ecliptic}}506 bytes (65 words) - 16:59, 11 January 2010
- Auto-populated based on [[Special:WhatLinksHere/Ecliptic]]. Needs checking by a human.579 bytes (76 words) - 16:10, 11 January 2010
- {{r|Ecliptic}}556 bytes (69 words) - 11:49, 11 January 2010
- {{r|Ecliptic}}556 bytes (73 words) - 12:52, 22 February 2011
- |'''Inclination to ecliptic''':1 KB (126 words) - 00:49, 30 November 2011
- {{r|Ecliptic}}774 bytes (101 words) - 18:00, 11 January 2010
- {{r|Ecliptic}}969 bytes (130 words) - 18:34, 11 January 2010
- ...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 (556 words) - 15:10, 2 December 2010
- ...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 (618 words) - 16:49, 28 November 2010
- {{r|Ecliptic}}2 KB (303 words) - 20:42, 11 January 2010
- {{r|Ecliptic}}2 KB (310 words) - 21:24, 11 January 2010
- ...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 (651 words) - 19:05, 9 February 2010
- ...the north pole) and it is this pole and its tilt with respect to the North Ecliptic Pole which determines the angle. In any case, my copy of the Encyclopedia o5 KB (895 words) - 23:55, 29 November 2011