Image:Main belt i vs a.png

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[edit] Summary

Description
English: Plot of inclination i vs semi-major axis a for numbered asteroids inward of about 6 AU. The main belt region is shown in red, and contains 93.4% of all the objects.

For reference, Mars orbits out to 1.666 AU, and Jupiter between 4.95 and 5.46 AU.

The diagram was created by Piotr Deuar [1] using orbit data for 120437 numbered minor planets from the Minor Planet Center orbit databse, dated 8 Feb 2006.
Source

http://en.wikipedia.org/wiki/Image:Main_belt_i_vs_a.png
Date

18:12, 2006-02-20
Author

Piotr Deuar
Permission
(Reusing this image)

see below

[edit] Licensing

GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation license, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled "GNU Free Documentation license".

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[edit] Original upload log

  • 17:47, 4 December 2006 Deuar (Talk | contribs | block) 1,280×929 48 KB modified version which distinguishes main belt/core region/rest
  • 18:12, 20 February 2006 Deuar (Talk | contribs | block) 1,201×901 44 KB

Historique du fichier

Cliquer sur une date et une heure pour voir le fichier tel qu’il était à ce moment-là

Date et heureDimensionsUtilisateurCommentaire
actuel18 janvier 2008 à 14:581 067×834 (19 Kio)Papa November (Language neutralised. No copyright claimed for non-creative derivative work)
18 janvier 2008 à 14:181 067×834 (20 Kio)Papa November (Rm opaque background, tight cropped and reduced to web colour palette using GIMP. No copyright claimed for non-creative derivative work)
26 août 2006 à 22:111 201×901 (44 Kio)Centaurus ({{Information |Description=Plot of inclination vs semi-major axis for numbered asteroids inward of about 6 AU. The main belt region is shown in red, and contains 93.4% of all the objects. For reference, Mars orbits out to 1.666 AU, and Jupiter between 4.)

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