Talk:Geology of Mercury
From Wikipedia, the free encyclopedia
 |
This article is within the scope of the Solar System WikiProject, a collaborative effort to improve Wikipedia's coverage of the Solar System. |
| B | This article has been rated as B-Class on the assessment scale. |
 |
Geology of Mercury is part of WikiProject Geology, an attempt at creating a standardized, informative, comprehensive and easy-to-use geology resource. If you would like to participate, you can choose to edit this article, or visit the project page for more information. |
| B | This article has been rated as B-class on the quality scale. |
| High | This article has been rated as high-importance on the importance scale. |
You guys hardly left any for me to translate :). In the "Origin of the planet's high luminosity and the presence of ice" section, the article stated that 2.4 GHz SHF waves were used to make a radar map of Mercury's surface. AFAIK (and our own EM spectrum article agrees) 2.4 GHz falls into the UHF band, so I changed that. Another great translation, guys! Fernando Rizo 30 June 2005 00:57 (UTC)
