File:North pole of Venus.jpg

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English: The Magellan probe that orbited Venus from 1990 to 1994 was able to peer through the thick Venusian clouds and build up the above image by emitting and re-detecting cloud-penetrating radar. Visible as the bright patch below central North is Venus' highest mountain Maxwell Montes. Other notable features include numerous mountains, coronas, impact craters, tessera, ridges, and lava flows. Although the size and mass of Venus are similar to the Earth, its thick carbon-dioxide atmosphere has trapped heat so efficiently that surface temperature usually exceeds 700 kelvins, hot enough to melt lead.
Date between 1990 and 1994
date QS:P,+1990-00-00T00:00:00Z/8,P1319,+1990-00-00T00:00:00Z/9,P1326,+1994-00-00T00:00:00Z/9
Source http://img1.wikia.nocookie.net/__cb20140701041517/solarsystemtour/images/c/ce/North_pole_of_Venus.jpg
Author NASA/JPL, SSV, MIPL (image processed by Jcpag2010)

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current02:20, 3 July 2014Thumbnail for version as of 02:20, 3 July 20141,000 × 960 (1.09 MB)Jcpag2012 (talk | contribs){{Information |Description ={{en|1=The Magellan probe that orbited Venus from 1990 to 1994 was able to peer through the thick Venusian clouds and build up the above image by emitting and re-detecting cloud-penetrating radar. Visible as the bright pa...

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