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Orbital pole






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From Wikipedia, the free encyclopedia
 


This is an old revision of this page, as edited by Bryan Derksen (talk | contribs)at08:36, 17 December 2005 (initial article to hold an orphaned image, also using text copied from Prograde and retrograde motion). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
(diff)  Previous revision | Latest revision (diff) | Newer revision  (diff)

File:Poles.png
The orbital poles of the Solar system. The yellow dot in the centre is the Sun's North pole. Jupiter's orbital pole is in orange, Mercury in pale blue, Venus in green, Earth in blue, Mars in red, Saturn in violet, Uranus in grey and Neptune in lavender. Pluto is the dotless cross off in Cepheus

Anorbital pole is either end of an imaginary line running through the center of an orbit perpendicular to the orbital plane. It is similar in concept to a geographical pole but based on the planet's orbit instead of the planet's rotation.

The north orbital pole of a celestial body is defined by the right-hand rule: If you curve the fingers of your right hand along the direction of orbital motion, with your thumb extended parallel to the orbital axis, the direction your thumb points is defined to be north.

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    This page was last edited on 17 December 2005, at 08:36 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



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