Asteroid_osculating_vs_proper_elements.png
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Summary
Description Asteroid osculating vs proper elements.png |
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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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 . Subject to disclaimers . http://www.gnu.org/copyleft/fdl.html GFDL GNU Free Documentation License true true |
Original upload log
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- 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