File:Solar System Venus 2012 transit.svg
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DescriptionSolar System Venus 2012 transit.svg | Location of planets of the Solar System, Pluto, Ceres and Halley's Comet viewed perpendicular to the ecliptic directly above the Sun during the transit of Venus on 5-6 June 2012; planet sizes are to scale, and planet orbits are to (a different) scale. Constellations names correspond to directions to constellations along the ecliptic. Brighter parts of orbits are nearer to the viewer than the ecliptic and darker parts are farther. Data was compiled from [1] Note: The MediaWiki SVG renderer does not support stroke-dashoffset so brighter/darker parts of orbits are shifted. Click the image to see the original (correct) SVG. | ||||
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SVG InfoField | This SVG map uses required raster graphics to show delicate structures.
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I, the copyright holder of this work, hereby publish it under the following licenses:
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | ||
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This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue |
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.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
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Original upload log
[edit]This image is a derivative work of the following images:
- File:Solare_Planeten99.jpg licensed with Cc-by-sa-3.0-migrated, GFDL
- 2006-12-25T14:06:41Z Filemon 217x688 (23374 Bytes) Przywrócono starszą wersję
- 2006-11-25T19:58:35Z Marcin Suwalczan 189x599 (26085 Bytes) The Photos of the Planets are from the NASA-Site: {{PD-USGov-NASA}} The Image you see is my work: {{GFDL}} [[Category:Sol System planets]]
- 2006-08-28T06:35:19Z Thuresson 217x688 (23374 Bytes) Återgått till tidigare version
- 2006-08-28T00:59:27Z Egg 217x642 (12501 Bytes) Pluto cut off, it is not a planet.
- 2006-08-27T11:03:12Z Thuresson 217x688 (23374 Bytes) Återgått till tidigare version
- 2006-08-24T15:12:13Z Bjb-de 217x653 (31015 Bytes) Pluto isn't a planet any more
- 2004-11-16T22:56:14Z Horst Frank 217x688 (23374 Bytes) Solar Planets
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 21:57, 31 March 2011 | 512 × 512 (66 KB) | Cmglee (talk | contribs) | Reverted to version as of 20:31, 31 March 2011 as giving up trying to fix orbits | |
21:55, 31 March 2011 | 512 × 512 (66 KB) | Cmglee (talk | contribs) | Check if path arcs work. | ||
20:31, 31 March 2011 | 512 × 512 (66 KB) | Cmglee (talk | contribs) | Try to fix stroke-dasharray. | ||
18:58, 29 March 2011 | 512 × 512 (66 KB) | Cmglee (talk | contribs) | Fix MediaWiki rendering by not using stroke-dashoffset attribute. | ||
05:14, 29 March 2011 | 512 × 512 (65 KB) | Cmglee (talk | contribs) | Add Halley's comet. | ||
12:02, 28 March 2011 | 512 × 512 (64 KB) | Cmglee (talk | contribs) | Fix bitmaps invisible in Firefox 3.5.18, text rotation and colours. | ||
00:08, 28 March 2011 | 512 × 512 (64 KB) | Cmglee (talk | contribs) | Realign text. | ||
22:43, 27 March 2011 | 512 × 512 (64 KB) | Cmglee (talk | contribs) | Fix radial gradients for librsvg renderer. | ||
22:41, 27 March 2011 | 512 × 512 (64 KB) | Cmglee (talk | contribs) | Complete illustration. | ||
15:54, 27 March 2011 | 512 × 768 (18 KB) | Cmglee (talk | contribs) | {{Information |Description=Location of planets of the Solar System during the transit of Venus on 5-6 June 2012; planet sizes are to scale, and planet orbits are to (a different) scale. |Source=*File:Solare_Planeten99.jpg |Date=2011-03-27 15:52 (UTC |
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Short title | Map of planets of the Solar System during the transit of Venus on 5-6 June 2012 |
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Image title | Map of planets of the Solar System, Halley's Comet, Pluto and Ceres during the transit of Venus on 5-6 June 2012, viewed perpendicular to the ecliptic directly above the Sun. Brighter parts of orbits are nearer to the viewer than the ecliptic and darker parts are farther. Planet sizes are to scale,and orbits are to (a different) scale. Data compiled from http://fourmilab.ch/cgi-bin/Solar?utc=2012-6-6&date=1&imgsize=1024&hlon=-14&orb=-b1 by CMG Lee. |
Width | 100% |
Height | 100% |