File:Outersolarsystem objectpositions labels comp-fr.png

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English: Legend

Axes list distances in AU, projected onto the ecliptic, with ecliptic longitude zero being to the right, along the "x" axis).

Positions are accurate for January 1st, 2000 (J2000 epoch) with some caveats: For planets, positions should be exact. For minor bodies, positions are extrapolated from other epochs assuming purely Keplerian motion. As all data is from an epoch between 1993 and 2007, this should be a reasonable approximation.

Data from the Minor Planet Center[1] or Murray and Dermott[2] as needed.

In the Kuiper Belt, radial "Spokes" of higher density, or gaps in particular directions are due to observational bias (i.e. where objects were searched for), rather than any real physical structure.

References

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  1. ↑ The MPC Orbit (MPCORB) Database.
  2. ↑ Carl D. Murray and Stanley F. Dermott (1999) Solar System Dynamics, Cambridge University Press ISBN: 0 521 57295.9. ISBN: 0 521 57295.9
Description
Français : Les « rayons » radiaux de densité plus élevée de cette image, ou les lacunes dans des directions particulières, sont dus au biais d'observation (lieux où l'on a recherché des objets) plutôt qu'à une quelconque structure physique réelle.
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Source Image:Outersolarsystem objectpositions labels comp.png from Wikimedia Commons, made and uploaded by WilyD, licensed same as this picture (see below).
Author WilyD
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This text courtest User:WilyD, User:Deuar and User:Serendipodous, all of the English Wikipedia. Consequently, while the image is released under the above licenses, the text is GFDL only.

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