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File:Vulcanoidorbits.png

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Vulcanoidorbits.png(600 × 600 pixels, file size: 37 KB, MIME type: image/png)

Summary

Description

The gravitationally stable zone in which Vulcanoid asteroids might exist

Date
Source I created this work entirely by myself.
Author Reyk YO!

Licensing

Public domain This work has been released into the public domain by its author, Reyk. This applies worldwide.
In some countries this may not be legally possible; if so:
Reyk grants anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law.

Original upload log

The original description page was here. All following user names refer to en.wikipedia.

Upload date | User | Bytes | Dimensions | Comment

  • 2009-01-05 00:37:54 | Reyk | 37429 | 600×600 | The vulcanoid zone, compared with the orbits of Mercury, Venus and Earth
  • 2008-12-26 21:59:34 | Reyk | 34673 | 600×600 | Reverted to version as of 21:56, 26 December 2008
  • 2008-12-26 21:59:09 | Reyk | 34673 | 600×600 | The vulcanoid zone, compared with the orbits of Mercury, Venus and Earth
  • 2008-12-26 21:56:43 | Reyk | 34673 | 600×600 | The Vulcanoid zone, compared with the orbits of Mercury, Venus and the Earth
  • 2008-12-25 12:31:15 | Reyk | 35929 | 600×600 | {{Information |Description=The gravitationally stable zone in which Vulcanoid asteroids might exist |Source=I created this work entirely by myself. |Date=2008-12-25 |Author=~~~ |other_versions= }}

File history

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Date/TimeThumbnailDimensionsUserComment
current15:49, 27 August 2013Thumbnail for version as of 15:49, 27 August 2013600 × 600 (37 KB)Szczureq== Summary == {{Information |Description = The gravitationally stable zone in which Vulcanoid asteroids might exist |Source = I created this work entirely by myself. |Date = 2008-12-25 |Author = <font color="Maroon">'''Reyk'''</font> {{C...
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