Venus is one of the four
terrestrial planets in the Solar System, meaning that it is a rocky body like Earth. It is similar to Earth in size and mass and is often described as Earth's "sister" or "twin". The surface pressure is , and the average surface temperature is , above the
critical points of both major constituents and making the surface atmosphere a
supercritical fluid of mainly
supercritical carbon dioxide and some supercritical nitrogen.
Natural history Formation The rocky terrestrial planets including Venus are thought to have formed in 5 stages: dust settling,
planetesimal formation, planetary embryos, giant impacts, and finally formation of atmospheres. Limited measurements from Venus have prevented a more detailed analysis of the formation timeline.
Future Venus is expected to be destroyed, along with Mercury, and possibly the Earth and the Moon, when the Sun becomes a
red giant in approximately seven or eight billion years.
Geography The Venusian surface was a subject of speculation until some of its secrets were revealed by probes in the 20th century.
Venera landers in 1975 and 1982 returned images of a surface covered in sediment and relatively angular rocks. such as flows on
Sif Mons, a shield volcano, and on
Niobe Planitia, a flat plain. However, the nature of tessera terrains is far from certain. Venus has gained interest as a case for research into the development of
Earth-like planets and
their habitability.
Volcanism s in Venus's Eistla region—both wide and less than high Much of the Venusian surface appears to have been shaped by volcanic activity. Venus has several times as many volcanoes as Earth, and it has 167 large volcanoes that are over across. The only volcanic complex of this size on Earth is the
Big Island of Hawaii. This is not because Venus is more volcanically active than Earth, but because its crust is older and is not subject to the
erosion processes active on Earth. Earth's
oceanic crust is continually recycled by
subduction at the boundaries of tectonic plates, and has an average age of about 100 million years, In 2008 and 2009, the first direct evidence for ongoing volcanism was observed by
Venus Express, in the form of four transient localized infrared hot spots within the rift zone
Ganis Chasma,
Craters s on the surface of Venus (false-colour,
3D projection image reconstructed from radar data) There are almost a thousand impact craters on Venus, evenly distributed across its surface. On other cratered bodies, such as Earth and the Moon, craters show a range of states of degradation. On the Moon, degradation is caused by subsequent impacts, whereas on Earth it is caused by wind and rain erosion. On Venus, about 85% of the craters are in pristine condition. The number of craters, together with their well-preserved condition, indicates the planet underwent a global resurfacing event 300–600million years ago, The principal difference between the two planets is the lack of evidence for plate tectonics on Venus, possibly because its crust is too strong to
subduct without water to make it less
viscous. This results in reduced heat loss from the planet, preventing it from cooling and providing a likely explanation for its lack of an internally generated
magnetic field. The weak magnetosphere around Venus means that the solar wind interacts directly with its outer atmosphere. Here, ions of hydrogen and oxygen are being created by the
dissociation of water molecules due to
ultraviolet radiation. The solar wind then supplies energy that gives some of these ions sufficient speed to escape Venus's gravity field. This erosion process results in a steady loss of low-mass hydrogen, helium, and oxygen ions, whereas higher-mass molecules, such as carbon dioxide, are more likely to be retained. Atmospheric erosion by the solar wind could have led to the loss of most of Venus's water during the first billion years after it formed. However, the planet may have retained a dynamo for its first 2–3 billion years, so the water loss may have occurred more recently. The erosion has increased the ratio of higher-mass
deuterium to lower-mass hydrogen in the atmosphere 100 times compared to the rest of the solar system. == Atmosphere and climate ==