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File:Main belt e vs a.png

Original file (1,086 × 834 pixels, file size: 55 KB, MIME type: image/png)

Summary

Description
English: Plot of eccentricity e vs en:semi-major axis a for numbered en:asteroids inward of about 6 AU. The en:main belt is shown in red and blue, and contains 98.5% of all the objects. Within this, the "core" region between the 4:1 and 2:1 en:Kirkwood gaps, and at moderate inclinations and eccentricities is shown in red. It contains 93.4% of all the objects.

For reference, en:Mars orbits out to 1.666 AU, and en:Jupiter between 4.95 and 5.46 AU.

The diagram was created by me (Piotr Deuar) using orbit data for 120437 numbered minor planets from the Minor Planet Center orbit databse, dated 8 Feb 2006.
Date 20 February 2006 (original upload date)
Source
English: Originally from en.wikipedia; description page is/was here.
Author Deuar at English Wikipedia
Other versions
This graph image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with {{vector version available|new image name}}.


It is recommended to name the SVG file “Main belt e vs a.svg”—then the template Vector version available (or Vva) does not need the new image name parameter.

Licensing

Note: "subject to disclaimers" below may not actually apply. This file was tagged with {{GFDL-user-en}}, and after May 2007, Template:GFDL-self (on English Wikipedia) did not require disclaimers. Please check the image description page on the English Wikipedia (or, if it has been deleted, ask an English Wikipedia administrator). See Wikipedia:GFDL standardization for details.

Exact dates for disclaimers to apply
Anything uploaded on the English Wikipedia with Template:GFDL-self within the following dates has disclaimers applicable. Otherwise, no disclaimers are applicable.
  • 22:43, 20 February 2004 to 17:19, 25 November 2005
  • 23:00, 26 November 2005 to 23:28, 18 May 2007
  • 21:17, 19 May 2007 to 20:01, 21 May 2007
For Template:GFDL, the dates are slightly different:
  • 21:43, 20 February 2004 to 16:27, 10 May 2007
Deuar at the English-language Wikipedia, the copyright holder of this work, hereby publishes it under the following license:
GNU head 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.

Note: This tag should not be used. For images that were released on the English Wikipedia using either GFDL or GFDL-self with disclaimers, use {{GFDL-user-en-with-disclaimers}}. For images without disclaimers please use {{GFDL-user-en-no-disclaimers}} instead. If you are the copyright holder of files that were released on Wikipedia, please consider removing the disclaimers.

Original upload log

(All user names refer to en.wikipedia)

  • 2006-12-04 17:53 Deuar 1280×929×8 (53535 bytes) modified version which distinguishes main belt/core region/rest
  • 2006-02-20 18:27 Deuar 1201×901×8 (50230 bytes)

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20 February 2006

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Date/TimeThumbnailDimensionsUserComment
current13:57, 18 January 2008Thumbnail for version as of 13:57, 18 January 20081,086 × 834 (55 KB)Papa Novemberrm deleted text artifacts with GIMP. No copyright claimed for non-creative derivative work
13:56, 18 January 2008Thumbnail for version as of 13:56, 18 January 20081,086 × 834 (55 KB)Papa NovemberRemoved opaque background, tight cropped and internationalised with GIMP. No copyright claimed for non-creative derivative work
03:16, 15 April 2007Thumbnail for version as of 03:16, 15 April 2007800 × 581 (139 KB)Dronemvp~commonswiki{{Information |Description=Plot of eccentricity vs en:semi-major axis for numbered en:asteroids inward of about 6 AU. The en:main belt is shown in red and blue, and contains 98.5% of al

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