File:TheKuiperBelt 550AU ESDO.svg

Original file (SVG file, nominally 800 × 400 pixels, file size: 31 KB)
Captions
Captions
Summary
editDescriptionTheKuiperBelt 550AU ESDO.svg |
Español: Objetos del disco difuso y del disco difuso extendido.
Extended Scattered Disk objects. Generated by a program written by Eurocommuter. |
Date | 20 February 2006 (original upload date) |
Source | No machine-readable source provided. Own work assumed (based on copyright claims). |
Author | No machine-readable author provided. Eurocommuter~commonswiki assumed (based on copyright claims). |
Main graph
editThe position of an object represents
- its orbit’s semi-major axis a in AU (horizontal axis)
- orbit’s inclination i in degrees (vertical axis).
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.
Main resonances with Neptune are marked with vertical bars; 1:1 marks the position of Neptune’s orbit (and its Trojan asteroids), 2:3 marks the orbit of Pluto (and its moons) etc.
Histograms
editHistograms show the population of objects with the parameter (eccentricity e and inclination i respectively) inside the given interval. The population is expressed in % of the total population (vertical axis)
- for inclination, the interval is 5o, i.e. the first bar shows the relative population of objects with i in 0-5o range, the next in 5-10o range etc.
- for the eccentricity e, the interval is 0.1, i.e. the first bar shows the relative population of objects with e in 0-0.1 range (quite circular orbits)
Data source
editMPCORB as of Feb 14th, 2006
Licensing
edit![]() |
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.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | |
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 22:00, 14 September 2006 | ![]() | 800 × 400 (31 KB) | Eurocommuter~commonswiki (talk | contribs) | Eris. |
22:05, 20 February 2006 | ![]() | 800 × 400 (35 KB) | Eurocommuter~commonswiki (talk | contribs) | Extended SDO. By Eurocommuter. Category:AstrophysicsCategory:Asteroids |
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