IMAGE 100_199\180.Lbm,Mariner 10's cameras took this picture of clouds in Venus's atmosphere in ultraviolet light in February 1974.
IMAGE 200_299\269.Lbm,A remarkable view of the surface of Venus obtained by Magellan's radar, showing rugged terrain on a plateau (Lakshmi Planum) in Ishtar Terra, one of the two big continents on the planet.
IMAGE 200_299\270.Lbm,A Magellan radar image of the surface of Venus, showing what appear to be a volcanic crater and lava flows.
IMAGE 200_299\271.Lbm,False-colour imagery has been used to enhance features in a Magellan radar scan of Venus. At bottom right is an impact crater, and surrounding flows of ejected material.
IMAGE 600_699\601.Lbm,A false-colour image of Venus, returned by the Pioneer-Venus orbiter, showing temperature variations. Venus's north pole is at the centre.
IMAGE 800_899\838.Lbm,Aphrodite Terra, one of the two 'continents' on Venus, compared in size with the USA.
IMAGE 1000_99\64.Lbm,Mosaic image of Venus produced from the radar scans by the orbiting Magellan probe in 1991. The view is centred at 90 degrees east longitude.
IMAGE 1000_99\65.Lbm,Mosaic image of Venus produced from scans by Magellan's radar in 1991. The view is centred at 0 degrees east longitude.
IMAGE 1000_99\66.Lbm,A computer-simulated view of the surface of Venus, based on radar scans by Magellan in 1991. It shows a volcanic crater with a diameter of about 25 km, surrounded by numerous lava flows.
