File:TheTransneptunians 73AU.svg

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Contents

[edit] Summary in English

The distribution and classification of the trans-Neptunian Objects. Generated by a program written by Eurocommuter.

Trans-Neptunian Objects (High Res)

See also the high resolution (richer content) version.

[edit] Main graph

The characteristics of an object in the graph represent:

  • Distance along horizontal axis
    • the object's orbital semi-major axis a in Astronomical Units
    • orbital period in years (in red)
  • Distance along vertical axis - the object's orbital inclination i in degrees
  • Size of the circle - the object’s size relative to others:
    • for a few large objects, the diameter drawn represents the best current estimates
    • for all the others, the diameter of the circle represents the absolute magnitude H of the object.
  • vertical bars mark orbital resonances with Neptune; 1:1 marks the position of Neptune’s orbit (and its Trojan asteroids), 2:3 marks the orbit of Pluto and plutinos.

[edit] Families

   Cubewanos
   Centaurs (not formally members of Trans-Neptunian objects, shown for reference only)
   Resonant objects - Plutinos and Resonant trans-Neptunian objects
   Scattered disc objects

To highlight other resonant objects, all of them are plotted in red.

[edit] Data source

Minor Planet Center Orbit database (MPCORB) as of 2008-10-05. Resonant orbits' classification from MPEC Circular 2008-S05 (2008-10-01). Diameter estimates include Stansberry et al (Spitzer). See refs in the related articles.

[edit] Description en français

La distribution et les familles des transneptuniens Graphique généré par un programme écrit par Eurocommuter.

[edit] Graphe principal

La position d’un objet représente

  • le demi axe majeur (rayon moyen) de son orbite a en in au (l’axe horizontal)
  • l’inclination de son orbite i en degrés (axe vertical).

Le diamètre du cercle montre la taille relative de l’objet aux autres. Pour quelques grands objets, le diamètre représente la meilleure estimation connue. Pour tous les autres, le diamètre du cercle représente la magnitude absolue de l’objet.

Les positions des résonances avec Neptune sont marqués par des traits verticaux; 1:1 marque la position de l’orbite de Neptune (et ses Troyens), 2:3 marque l’orbite de Pluton (et ses lunes) etc.

[edit] Familles

  • Centaures ne sont pas formellement membres des transneptuniens
  • La Ceinture de Kuiper regroupe
    • Objets classiques, cubewanos, en bleu
    • Objets résonants en 2:3 et 1:2, en rouge
  • Objets épars, en gris

Pour repérage facile tous les autres objets résonants sont en rouge.

[edit] Source des données

Base de données MPCORB au 1er decembre 2007, sauf pour la classification des orbites résonantes où le Minor Planet Circular 2007-W54 [1] a été utilisé.

[edit] Licensing

I, the copyright holder of this work, hereby publish it under the following licenses:
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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Creative Commons license
Creative Commons Attribution Creative Commons Share Alike
This file is licensed under the Creative Commons Attribution ShareAlike 2.5, Attribution ShareAlike 2.0 and Attribution ShareAlike 1.0 License. In short: you are free to share and make derivative works of the file under the conditions that you appropriately attribute it, and that you distribute it only under a license identical to this one.

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File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current05:54, 16 October 2008Thumbnail for version as of 05:54, 16 October 2008800×400 (116 KB)Eurocommuter (Talk | contribs) (Re-plotted from current MPC database. Added indication of orbital period. Category:Trans-Neptunian objects)
11:15, 20 September 2008Thumbnail for version as of 11:15, 20 September 20082,000×1,000 (118 KB)Chesnok (Talk | contribs) (naming Haumea and Makemake)
16:26, 26 March 2008Thumbnail for version as of 16:26, 26 March 20082,000×1,000 (118 KB)Chesnok (Talk | contribs) (A name of an asteroid must contain space between year and letters!)
15:40, 2 December 2007Thumbnail for version as of 15:40, 2 December 20072,000×1,000 (118 KB)Eurocommuter (Talk | contribs) (Fixed the viewbox.)
15:34, 2 December 2007Thumbnail for version as of 15:34, 2 December 20072,000×1,000 (118 KB)Eurocommuter (Talk | contribs) (Refreshed data sources. Orbits: MPCORB database 2007-12-01. Types: MPEC 2007-W54 (2007-11-22). Sizes: include Stansberry et al (Spitzer))
08:21, 9 March 2007Thumbnail for version as of 08:21, 9 March 20072,000×1,000 (114 KB)Eurocommuter (Talk | contribs) (Updated from MPCORB database 2007-03-07 and MPC Circ. Dec. 2006)
00:37, 18 November 2006Thumbnail for version as of 00:37, 18 November 20062,000×1,000 (121 KB)Augiasstallputzer (Talk | contribs) (Enlarged scale, for better text reading.)
08:44, 14 September 2006Thumbnail for version as of 08:44, 14 September 2006800×400 (121 KB)Eurocommuter (Talk | contribs) (Eris. Pluto demoted. Fixed stroke.)
10:00, 5 April 2006Thumbnail for version as of 10:00, 5 April 2006800×400 (122 KB)Eurocommuter (Talk | contribs) (Fixed MPC classification problem for Centaurs)
01:17, 23 February 2006Thumbnail for version as of 01:17, 23 February 2006800×400 (121 KB)Eurocommuter (Talk | contribs) (Trans-Neptunian Objects. By Eurocommuter.)

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