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Earth's cloudy "twin". Planet-wide swirls and waves appear in the thick atmosphere of Venus, as photographed by Pioneer Venus Orbiter. This view shows a pronounced dark band (lower left), two bright areas ("polar rings") near the north and south poles, and a complex, turbulent region at the left. These large-scale patterns are strikingly different from the numerous smaller circulation patterns of the Earth's atmosphere. The Venus patterns are remarkably stable and circle the planet in only four days, although the planet itself takes about 244 days to rotate on its axis. |
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Hot Rocks of Venus. Scorched to nearly red heat under the thick hot atmosphere of Venus, the planet's surface was photographed by two successful, but short-lived, Russian Venera landers. In this picture, jagged slabs of rock extend to the horizon (upper right). The nature of the rock is unknown. The images are curved by optical effects in the television cameras. Parts of the spacecraft are seen, out of focus, at lower center and lower right. |
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Highs and lows of Venus. This crude relief map of the cloud shrouded surface of Venus is based on radar observations made from Earth andfrom the Pioneer Venus Orbiter. Low elevations are shown in greens and blues, higher altitudes in yellows and reds. Most of Venus is much flatter than Earth, but a few plateaus the size of small continents rise up to 17 kilometers (11 miles) above their surroundings. There is no clear indication of anything resembling the global system of trenches and mid-ocean ridges that characterizes our geologically active Earth. |