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File:Asteroid osculating vs proper elements.png

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Summary

Description

osculating (Keplerian) zh:orbital elements (left) versus zh:proper orbital elements (right) for numbered zh:asteroids in the zh:main belt. The plots are of zh:inclinations i against eccentricities e.

Clumps in the (right) plot of proper orbital elements indicate the location of asteroid families, while they are almost indistinguishable in the (left) plot of standard Keplerian orbital elements.

This diagram was created by me (Piotr Deuar).

The right plot is a reduced version of zh::Image:Asteroid_proper_elements_i_vs_e.png, an image made using data for 96944 zh:minor planets that was obtained from the AstDys site. This data was dated March 2005, and computed by Z. Knezevic and A. Milani.

The left plot uses Keplerian orbital element data for the same 96944 minor planets taken from the astorb database. This data was dated 27 Dec 2005, and computed by Edward Bowell.
Date 21 May 2007 (original upload date)
Source Transferred from zh.wikipedia to Commons.
Author 凌雲 at Chinese Wikipedia

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Original upload log

The original description page was here. All following user names refer to zh.wikipedia.
  • 2007-05-21 09:40 凌雲 1200×450×4 (93860 bytes) {{Move to Commons}} {{Convert to SVG}} == Summary == [[Osculating orbit|osculating]] (Keplerian) [[orbital elements]] (''left'') versus [[proper orbital elements]] (''right'') for numbered [[asteroid]]s in the [[main belt]]. The plots are of [[inclinatio

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current04:36, 11 July 2007Thumbnail for version as of 04:36, 11 July 20071,200 × 450 (92 KB)Wong128hk{{Information |Description=osculating (Keplerian) zh:orbital elements (''left'') versus zh:proper orbital elements (''right'') for numbered zh:asteroids in the zh:main belt. The plots are of zh:inclination

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