Arecibo-GBT Image of Venus

This is a radar image of the planet Venus made by transmitting a signal at 13 cm wavelength from Arecibo and using the GBT to detect the reflection off its surface. Brighter parts of the image indicate a rougher surface, while dark regions are smoother (on centimeter to meter scales). Many features, including mountain ranges, volcanic domes, and craters can be seen. The resolution of this image varies from 1 to 5 km. Investigator(s): Donald Campbell, Jean-Luc Margot, Lynn Carter, and Bruce Campbell
Credit: Campbell et al., (NRAO/AUI/NSF); NAIC
Technical Details | |
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Telescope | GBT; Arecibo |
Band | S; S |
Date | 2001-00-00; 2001-00-00 |
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