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Venus (planet)

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Global view of the surface of Venus centered at 180 degrees east longitude

Click image for description
Orbital characteristics
Avg Dist from Sol AU
Mean radius 108,208,930 km
Eccentricity 0.00677323
Orbital period 224.695434 days
(0.6151826 yearss)
Synodic period 583.92 days
Avg. Orbital Speed 35.0214 km/s
Inclination 3.39471°
Number of satellitess 0
Physical characteristics
Equatorial diameter 12,103.6 km
Surface area 4.60×108 km2
Mass 4.869×1024 kg
Mean density 5.24 g/cm3
Equatorial gravity m/s2
Rotation period retrograde motion
Axial tilt 2.64°
Albedo 0.65
Escape Speed 10.36 km/s
Surface* temp
min* mean max
K 737 K 773 K
(*min temperature refers to cloud tops only)
Atmospheric characteristics
Atmospheric pressure kPa
Carbon dioxide 96%
Nitrogen 3%
Sulfur dioxide
Water vapor
Carbon monoxide
Carbonyl sulfide
Hydrogen chloride
Hydrogen fluoride

Venus is the second planet from the Sun, named after the Roman goddess Venus. It is a terrestrial planet, very similar in size and bulk composition to Earth; it is sometimes called Earth's "sister planet" as a result of this similarity.

Because Venus is closer to the Sun than Earth is, it is always in roughly the same direction as the Sun, so on Earth it can only be seen just before sunrise or just after sunset. It is sometimes referred to as the "morning star" or the "evening star", and when it appears it is by far the brightest point of light in the sky.

Table of contents
1 Physical characteristics
2 Exploration of Venus
3 Venus in fiction
4 See also
5 External links

Physical characteristics


Venus has an atmosphere consisting mainly of carbon dioxide and a small amount of nitrogen, with a pressure at the surface about 90 times that of Earth (a pressure equivalent to a depth of 1 kilometer under Earth's ocean). This enormous CO2-rich atmosphere results in a strong greenhouse effect that raises the surface temperature approximately 400°C above what it would be otherwise, causing temperatures at the surface to reach 500°C. This makes Venus's surface hotter than Mercury's, despite being nearly twice as distant from the Sun and only receiving 25% the solar irradiance (2613.9 W/m² in the upper atmosphere, and just 1071.1 W/m² at the surface). Due to the thermal inertia and convection of its dense atmosphere, the temperature does not vary significantly between the night and day sides of Venus despite its extremely slow rotation (less than one rotation per Venusian year; at the equator, Venus' surface rotates at a mere 4 miles per hour). Winds in the upper atmosphere circle the planet in only 4 days, helping to distribute the heat.

Venus shrouded in thick clouds, shown through ultraviolet filtersEnlarge

Venus shrouded in thick clouds, shown through ultraviolet filters

There are strong 350-kilometer-per-hour winds at the cloud tops but winds at the surface are very slow, no more than a few kilometers per hour. However, due to the high density of the atmosphere at Venus's surface, even such slow winds exert a significant amount of force against obstructions. The clouds are composed of sulfur dioxide and sulphuric acid droplets and cover the planet completely, obscuring any surface details. The temperature at the tops of these clouds is approximately -45°C. The official mean surface temperature of Venus, as given by NASA, is 464°C. The minimal value of the temperature, listed in the table, refers to cloud tops—on surface the temperature is never below 400°C.

Surface features

Venus has slow retrograde rotation, meaning it rotates from east to west instead of west to east as most of the other major planets. (Pluto and Uranus also have retrograde rotation, though Uranus' axis, tilted at 97.86 degrees, almost lies in its orbital plane.) It is not known for sure why Venus is different in this manner, although it may be the result of a collision with a very large asteroid at some time in the distant past. In addition to this unusual retrograde rotation, the periods of Venus's rotation and of its orbit are synchronized in such a way that it always presents the same face toward Earth when the two planets are at their closest approach (5.001 Venusian days between each inferior conjunction). This may be the result of tidal locking, with tidal forces affecting Venus's rotation whenever the planets get close enough together, or it may simply be a coincidence.

Venus has two major continent-like highlands on its surface, rising over vast plains. The northern highland is named Ishtar Terra and has Venus's highest mountains, named the Maxwell Montes (roughly 2km taller than Mount Everest) after James Clerk Maxwell, which surround the plateau Lakshmi Planum. Ishtar Terra is about the size of Australia. In the southern hemisphere is the larger Aphrodite Terra, about the size of South America. Between these highlands are a number of broad depressions, including Atalanta Planitia, Guinevere Planitia, and Lavinia Planitia. With only the exception of Maxwell Montes, all surface features on Venus are named after real or mythological females. Due to Venus's thick atmosphere, which causes meteors to decelerate as they fall toward the surface, no impact crater smaller than about 3.2 km in diameter can form.

Nearly 90% of Venus's surface appears to consist of recently-solidified basalt lava, with very few meteor craters. This suggests that Venus underwent a major resurfacing event recently. The interior of Venus is probably very similar to that of Earth: an iron core about 3000 km in radius, with a molten rocky mantle making up the majority of the planet. Recent results from the Magellan gravity data indicate that Venus's crust is stronger and thicker than had previously been assumed. It is theorized that Venus does not have mobile plate tectonics like Earth does, but instead undergoes massive volcanic upwellings at regular intervals that inundate its surface with fresh lava; the oldest features present on Venus seem to be only around 800 million years old, with most of the terrain being considerably younger (though still not less than several hundred million years for the most part). Recent findings suggest that Venus is still volcanically active in isolated geological hot spots.

Venus has no magnetic field, possibly due to its slow rotation being insufficient to drive an internal dynamo of liquid iron. As a result, the solar wind impacts directly on Venus's upper atmosphere. It is thought that Venus originally had as much water as Earth, but that under the Sun's assault water vapor in the upper atmosphere was split into hydrogen and oxygen, with the hydrogen escaping into space due to its low molecular mass; the ratio of hydrogen to deuterium (a heavier isotope of hydrogen which doesn't escape as quickly) in Venus's atmosphere seems to support this theory. The oxygen is thought to have combined with atoms in the crust and disappeared from the atmosphere.

Venus was once thought to possess a moon, named Neith after the mysterious goddess of Sais (whose veil no mortal raised), first observed by Giovanni Domenico Cassini in 1672. Sporadic sightings of Neith by astronomers continued until 1892, but these sightings have since been discredited (they were mostly faint stars that happened to be in the right place at the right time) and Venus is now known to be moonless.

Exploration of Venus

Historical observations

Venus is the most prominent astronomical feature in the morning and evening sky on Earth (besides the Sun and Moon), and has been known of since before recorded history. One of the oldest surviving astronomical documents, from the Babylonian library of Ashurbanipal around 1600 BC, is a 21-year record of the appearances of Venus (which the early Babylonians called Nindaranna). The ancient Sumerians and Babylonians called Venus Dil-bat or Dil-i-pat; in Akkadia it was the special star of the mother-god Ishtar; and in Chinese it is the god Jin xing. Venus was the most important celestial body observed by the Maya, who called it Chak ek, "the Great Star", and considered it a representation of Quetzalcoatl; they apparently did not worship any of the other planets. (See also Maya calendar.)


Phases of VenusEnlarge

Phases of Venus


Transits of Venus, when the planet crosses directly between the Earth and the Sun' visible disc, are rare astronomical events. The first time such a transit was observed was on December 4, 1639 by Jeremiah Horrocks and William Crabtree. A transit in 1761 observed by Mikhail Lomonosov provided the first evidence that Venus had an atmosphere, and the 19th century observations of parallax during its transits allowed the distance between the Earth and Sun to be accurately calculated for the first time. The previous set of transits of Venus occurred within the interval of 18741882, and the next set of transits will occur in the period of 20042012.

In the 19th century, many observers stated that Venus had a period of rotation of roughly 24 hours. Italian astronomer Giovanni Schiaparelli was the first to predict a significantly slower rotation, proposing that Venus was tidally locked with the Sun (as he had also proposed for Mercury). While not actually true for either body, this was still a reasonably accurate estimate. The near-resonance between its rotation and its closest approach to Earth helped to create this impression, as Venus always seemed to be facing the same direction when it was in the best location for observations to be made. The rotation rate of Venus was finally determined with confidence in 1961, using the Goldstone Radio Telescope in California. The fact that it was retrograde was not confirmed until 1964, however.

Before detailed observations, many believed that Venus contained a lush, earth-like environment. Scientists cited the planet's size and orbital radius, which presented a fairly earth-like situation. Soon after though an accurate composition of the planet's atmosphere was deduced, and theories of a habitable Venus were discarded.

Venus-observation spacecraft

Color image taken from the surface of Venus by the Soviet Venera 13 landerEnlarge



The first successful Venus probe was the American Mariner 2 spacecraft, which flew past Venus in 1962. It established that Venus has no magnetic field and measured the planet's rotation rate. In the late 1970's NASA sent two Pioneer spacecraft to Venus. The Pioneer mission consisted of two components, launched separately: an Orbiter and a Multiprobe. The Pioneer Venus Multiprobe carried one large and three small atmospheric probes. The large probe was released on November 16, 1978 and the three small probes on November 20. All four probes entered the Venus atmosphere on December 9, followed by the delivery vehicle. Although not expected to survive the descent through the atmosphere, one probe continued to operate for 45 minutes after reaching the surface. The Pioneer Venus Orbiter was inserted into an elliptical orbit around Venus on December 4, 1978. It carried 17 experiments and operated until the fuel used to maintain its orbital position was exhausted and atmospheric entry destroyed the spacecraft in August, 1992.

The Soviet Union sent a number of atmospheric probes and landers, with Venera 9 and 10 each returning a single black-and-white photograph of Venus's surface in 1975 and Venera 13 and 14 returning a number of color photographs from Venus's surface in 1982. In 1985 the Soviet Vega 1 and 2 probes each deployed a sensor-laden balloon in Venus's atmosphere in addition to placing landers on the surface. No lander survived for more than about two hours before failing under Venus's intense surface heat and pressure.

Venus's 2004 transit across the Sun
On August 10, 1990, the US Magellan probe arrived at its orbit around the planet and started a mission of detailed radar mapping. 98% of the surface was mapped with a resolution of approximately 100m before the craft, on October 11, 1994, plunged to the surface as planned and partly vaporized; some sections are thought to have hit the planet's surface.

Venus Express is a future mission proposed by the European Space Agency which would study Venus from orbit.

Venus in fiction

Until it was penetrated by probes, Venus's opaque cloud layer gave science fiction writers free reign in imagining the planet's surface, and they frequently imagined it to be Earth-like. Venus was the home planet of the Mekon, arch-enemy of the 1950s comic book hero Dan Dare, and was the site of a second garden of Eden in C. S. Lewis's novel Perelandra. Venus is also the location of several Starfleet Academy training facilities and terraforming stations in the fictional Star Trek universe, and is briefly mentioned in Arthur C. Clarke's .

See also

External links

The Solar System