Arecibo-GBT Image of Venus

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Arecibo-GBT Image of Venus

Radar image of half of the planet 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
Telescope	GBT; Arecibo
Band	S; S
Date	2001-00-00; 2001-00-00

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