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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 E
    2 KB (333 words) - 05:31, 24 March 2010
  • 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

Page text matches

  • [[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 E
    2 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]] and
    1 KB (214 words) - 13:01, 18 November 2022
  • ...[Spica]], and [[Regulus]] it is one of the four brightest stars near the [[ecliptic]]. The similarly-colored [[Aldebaran]] (α [[Taurus|Tauri]]) lies almost d
    507 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
  • {{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 orbit
    3 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 prec
    4 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 '''Tw
    5 KB (651 words) - 19:05, 9 February 2010
  • ...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 a
    8 KB (1,202 words) - 08:50, 10 January 2021
  • ...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.<r
    18 KB (2,977 words) - 10:50, 22 February 2023
  • ...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 to
    23 KB (3,632 words) - 18:47, 8 April 2014
  • ...Hipparchus discovered the equinoxes were not static, but move West on the ecliptic when compared to distant stars that relatively seem fixed at this distance.
    10 KB (1,472 words) - 08:34, 8 June 2009
  • ...ii]], and about [[Tau Sagittarii|3.5 degrees south]] of the [[plane of the ecliptic]]. [[Tau Sagittarii]] is the closest easily visible star.
    12 KB (1,817 words) - 22:07, 30 April 2013
  • ...rn] is surrounded by a thin, flat, ring, nowhere touching, inclined to the ecliptic." <ref>http://www2.jpl.nasa.gov/saturn/back.html</ref> ...akes approximately 29 and a half years to make a complete circuit of the [[ecliptic]] against the background constellations of the [[zodiac]]. Optical aid (a l
    23 KB (3,601 words) - 18:46, 13 January 2021
  • ...]] claim that the position of the planets within various sections of the [[ecliptic]] can be an indicator of events on Earth. By carefully measuring the orbits
    12 KB (1,829 words) - 10:07, 10 January 2021
  • ...plane parallel to that of Earth's orbit. The planets are very close to the ecliptic while [[comet]]s and [[kuiper belt]] objects are usually at significantly g ...ts the Sun on its side; its [[axial tilt]] is over ninety degrees to the [[ecliptic]]. It has a much colder core than the other gas giants, and radiates very l
    76 KB (11,605 words) - 21:48, 1 September 2020
  • ...is that this refers to a motion along the ecliptic or a description of the ecliptic with regard to twelve 30 degree signs which is connected with the zodiacal
    51 KB (8,075 words) - 05:28, 17 October 2013
  • ...esearch]] (NCAR) </ref> Galileo's geometric military compass, and Kepler's ecliptic instrument. Galileo not only had to adapt the telescope to astronomy, he al
    23 KB (3,546 words) - 19:39, 25 September 2020
  • ...top) and from the ascending node (below). The segments of orbits below the ecliptic are plotted in darker colours. The [[perihelion|perihelia]] (q) and [[aphe
    44 KB (6,986 words) - 09:16, 6 March 2024
  • ...inclination of Earth's [[equator|equatorial plane]] and the plane of the [[ecliptic]] relative to the galactic plane. The fact that the Milky Way divides the n
    37 KB (5,756 words) - 13:14, 10 January 2021
  • [[axial tilt|obliquity]] of the [[ecliptic]] was estimated as early as 1,000 B.C by the Chinese. The Chaldeans discove
    46 KB (6,796 words) - 10:08, 28 February 2024