File:TheKuiperBelt 55AU Classical.svg
Original file (SVG file, nominally 800 × 400 pixels, file size: 26 KB)
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Summary
[edit]DescriptionTheKuiperBelt 55AU Classical.svg |
English: Large classical Kuiper Belt objects (H<4.5).
The position of an object represents
The size of the circle illustrates the object’s size relative to others. For a few large objects, the diameter drawn represents the best current estimates. For all others, the circles represent the absolute magnitude of the object.
The eccentricity of the orbit is shown indirectly by a segment extending from the left (perihelion) to the aphelion to the right. In other words, the segment illustrates the variations of the object's distance from the Sun. Objects with nearly circular orbits will show short segments while highly elliptical orbits will be represented by long segments.
Français : Les grands objets classiques.
La position d’un objet représente
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. L’excentricité de l’orbite est représentée indirectement par un segment qui s’étend du périhélie à gauche) l’aphélie à droite. En d’autres termes, le segment illustre les variations de la distance du Soleil. Les objets avec des orbites quasi circulaires ont donc des courts segments et les orbites très excentriques sont repérées par des segments longs.Les positions des résonances avec Neptune sont marqués par des traits verticaux; 1:1 marque a position de l’orbite de Neptune (et ses Troyens), 2:3 marque l’orbite de Pluton (et ses lunes) etc. |
Date | 2006-02-17; updated 2007-03-22, 2008-10-19 |
Source |
Minor Planet Center Orbit database (MPCORB) as of 2008-10-05. (La base de donnés MPCORB au 14 Février 2006.) Orbits' classification from MPEC Circular 2008-S05 (2008-10-01) or from MPCORB. Diameter estimates include Stansberry et al. (Spitzer). See refs in the related articles. Plotted by a program written by the author |
Author | Eurocommuter~commonswiki |
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File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 11:00, 19 October 2008 | 800 × 400 (26 KB) | Eurocommuter~commonswiki (talk | contribs) | (aligned font with other graphs) | |
10:54, 19 October 2008 | 800 × 400 (24 KB) | Eurocommuter~commonswiki (talk | contribs) | Re-plotted from updated MPC database | ||
17:50, 23 September 2008 | 800 × 400 (14 KB) | Chesnok (talk | contribs) | 2003 EL61 = Haumea, 2005 FY9 = Makemake | ||
22:02, 22 March 2007 | 800 × 400 (15 KB) | Eurocommuter~commonswiki (talk | contribs) | Data source update after a year. | ||
12:12, 20 February 2006 | 800 × 400 (14 KB) | Eurocommuter~commonswiki (talk | contribs) | Large Classical Objects. Update by Eurocommuter | ||
11:28, 17 February 2006 | 800 × 400 (13 KB) | Eurocommuter~commonswiki (talk | contribs) | Large classical objects of the Kuiper Belt. Generated by a program written by Eurocommuter. |
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