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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This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: Make into solar system map during 2012 Venus transit. The original can be viewed here: Solare Planeten99.jpg: . Modifications made by Cmglee.
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Original upload log
This image is a derivative work of the following images:
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
{{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
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.