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Our knowledge concerning the surface of Venus comes from a limited amount of information obtained by the series of Russian Venera landers, and primarily from extensive radar imaging of the planet. The radar imaging of the planet has been performed both from Earth-based facilities and from space probes. The most extensive radar imaging was obtained from the Magellan orbiter in a 4-year period in the early 1990s. As a consequence, we now have a detailed radar picture of the surface of Venus. The adjacent animation shows the topography of the surface as determined using the Magellan synthetic aperture radar (black areas are regions not examined by Magellan). An MPEG movie (303 kB) of this animation is also available.

Overview of SurfaceThe surface of Venus is rather smooth in many places, though not nearly as smooth as originally expected . However, we find evidence for many of the same geological features found on Earth: canyons, volcanoes, lava flows, rift valleys, mountains, craters, and plains. There is substantial evidence for local tectonic activity but the surface appears to be a single crustal plate, with little evidence for large-scale horizontal motion of crustal plates as found on the Earth. Why the two planets differ in this aspect of their geology even though we believe them to have similar interiors is not well understood. The usual explanation is that Venus is a little behind the Earth in geological timescale, and its tectonic activity is just getting started.

Much of the surface of Venus appears to be rather young. The global data set from radar imaging reveals a number of craters consistent with an average Venus surface age of 300 million to 500 million years.

There are two "continents", which are large regions several kilometers above the average elevation. These are called Istar Terra and Aphrodite Terra. They can be seen in the preceding animation as the large green, yellow, and red regions indicating higher elevation near the equator (Aphrodite Terra) and near the top (Ishtar Terra).

Hemispheric ViewsThe following images show 5 hemispheric views of the surface, again as determined primarily from the Magellan mission.
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Related Questions

What is the composition of Venus' surface?

The surface of Venus is relatively smooth as it is believed that volcanic action has resurfaced the planet. The surface is composed of rock but we are uncertain exactly what type of rock. There is some evidence that there may be granite on Venus.


What is the topography and the surface of Venus?

The "topography" of Venus is the three dimensional shape of the surface of Venus.


What is the atmosphere on the surface of Venus's?

The atmosphere on the surface of Venus is cloudy.


Does venus have a solid surface or a surface made o f gases?

Venus has a solid rocky surface.


What is the description of venus?

Venus has craters on it's surface!


What are the surface appearance of planet Venus'?

The surface area of the planet Venus is 4.60×108 km2.


What kind of surface does Venus has?

Venus surface is a dry desertscape with many slab-like rocks


What are surface featurs of venus?

the surface feature of Venus are craters, meteorites and mostly acid water


Are there any pictures ever really been taken of the surface of Venus?

Yes, Go on the internet, go to google and type in "VENUS SUTRFACE" Go toimmages and their are some.Mr.Seidschlag


How can the surface of Venus' be observed with?

The surface of Venus can be observed using radar imaging from spacecraft orbiting the planet. Radar can penetrate through the thick clouds covering Venus and provide detailed images of its surface features. This method has been used by missions like NASA's Magellan spacecraft to map the surface of Venus.


Is gravity strong or weak in Venus?

It's roughly 10% less on the surface of Venus than on Earth's surface.


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Jupiter, at the surface anyway. Venus has the hottest surface temperature of all the planets.