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Venus

Webpages concerning "Venus"

Venus was named after the Roman goddess of love and beauty, but is now known to be very different from Earth. It has no oceans and is surrounded by a heavy atmosphere of carbon dioxide with clouds composed of sulfuric acid droplets.
http://www.solarviews.com/eng/venus.htm
Keywords:
venus, venusian, roman, goddess, of, love, roman goddess, jewel, of, the, sky, morning star, evening star, sister planet, planet, condensed, nebula, atmosphere, carbon dioxide, sulfuric acid, sulfuric acid clouds, atmospheric pressure, greenhouse, greenhouse effect, cloud deck, cloud, clouds, pioneer venus, venera, magellan, radar mapping, magellan radar mapping, nasa, spacecraft, map, mapping, ...

http://www.solarviews.com/eng/venus.htm

An in-depth factual look at the planet Venus, illustrated with pictures and information
http://www.solarspace.co.uk/Venus/venus.php
Keywords:
venus, hot, image, pictures, planet, life, sun, atmosphere, clouds, greenhouse effect, conditions, information, orbit, solar, description, text, fact, statistic

http://www.solarspace.co.uk/Venus/venus.php

Although Venus looks a lot like Earth. It's actually dramatically different.
http://csmonitor.com/2002/0510/p25s02-stss.html
Keywords:
Sci/Tech, Science & Space, Christian Science Monitor

http://csmonitor.com/2002/0510/p25s02-stss.html

Venus - Pictures and Astronomy Facts - Solar System Planetary Astronomical Data & Pictures of Venus. Venus. Astronomy Guide to Space exploration close to home. Venus whose Greek equivalent was Aphrodite was the Greek goddess of love and beauty. It probably got its name from being the brightest object in the sky except for the Sun & the Moon. At one time, it was thought to be two separate b...
http://space.about.com/od/venus/a/venusinfo.htm
Keywords:
venus, planet, solar, system, venus, astronomy, facts, pictures, venus, first, planet, 1st, planet

http://space.about.com/od/venus/a/venusinfo.htm

NSSDC Photo Gallery: Venus - A collection of images of the planet Venus
http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-venus.html
Keywords:
NASA, NSSDC, image, images, photo, photos, imagery, planet, planets, Venus

http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-venus.html

Venus, from ORRERY: the Solar System in action. Second closest planet to the Sun, yet the hottest!
http://www.harmsy.freeuk.com/venus.html
Keywords:
earth, longitude, john, harrison, Greenwich, andrew, harmsworth, orrery, planets, mercury, venus, weather, mars, jupiter, saturn, uranus, neptune, pluto, sun, asteroids, comets, education, science, space, kuiper belt, astronomy, photodesk

http://www.harmsy.freeuk.com/venus.html

http://www.windows.ucar.edu/tour/link=/venus/venus.html

http://www.windows.ucar.edu/tour/link=/venus/venus.html

http://www.nineplanets.org/venus.html

http://www.nineplanets.org/venus.html

http://www.cosmicelk.co.uk/Venus.htm

http://www.cosmicelk.co.uk/Venus.htm

http://csep10.phys.utk.edu/astr161/lect/venus/venus.html

http://csep10.phys.utk.edu/astr161/lect/venus/venus.html

http://www.mentallandscape.com/V_Venus.htm
Keywords:
Venus, Venera, Soviet, Space

http://www.mentallandscape.com/V_Venus.htm

http://pds.jpl.nasa.gov/planets/welcome/venus.htm

http://pds.jpl.nasa.gov/planets/welcome/venus.htm

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Wikipedia-Article "Venus"

For other uses, see Venus (disambiguation).
Venus Astronomical symbol of Venus
Venus

Click image for description

Orbital characteristics (Epoch J2000)
Semi-major axis 108,208,926 km
0.723 331 99 AU
Orbital circumference 0.680 Tm
4.545 AU
Eccentricity 0.006 773 23
Perihelion 107,476,002 km
0.718 432 70 AU
Aphelion 108,941,849 km
0.728 231 28 AU
Orbital period 224.700 69 d
(0.615 197 0 a)
Synodic period 583.92 d
Avg. orbital speed 35.020 km/s
Max. orbital speed 35.259 km/s
Min. orbital speed 34.784 km/s
Inclination 3.394 71°
(3.86° to Sun's equator)
Longitude of the
ascending node
76.680 69°
Argument of the
perihelion
54.852 29°
Number of satellites 0
Physical characteristics
Equatorial diameter 12,103.7 km
(0.949 Earths)
Surface area 4.60×108 km2
(0.902 Earths)
Volume 9.28×1011 km³
(0.857 Earths)
Mass 4.8685×1024 kg
(0.815 Earths)
Mean density 5.204 g/cm3
Equatorial gravity 8.87 m/s2
(0.904 gee)
Escape velocity 10.36 km/s
Rotation period -243.0185 d
Rotation velocity 6.52 km/h (at the equator)
Axial tilt 2.64°
Right ascension
of North pole
272.76° (18 h 11 min 2 s) 1
Declination 67.16°
Albedo 0.65
Surface* temp.
min* mean max
228 K 737 K 773 K
Adjective Venusian or (rarely) Cytherean
(*min temperature refers to cloud tops only)
Atmospheric characteristics
Atmospheric pressure 9.3 MPa
Carbon dioxide ~96.5%
Nitrogen ~3.5%
Sulfur dioxide .015%
Argon .007%
Water vapor .002%
Carbon monoxide .0017%
Helium .0012%
Neon .0007%
Carbonyl sulfide
Hydrogen chloride
Hydrogen fluoride
trace

Venus, the second planet from the Sun, is named after the Roman goddess Venus. A terrestrial planet, it is sometimes called Earth's "sister planet", as the two are very similar in size and bulk composition. Although all planets' orbits are elliptical, Venus's orbit is the closest to circular, with an eccentricity of less than 1%. As Venus is closer to the Sun than the Earth, it always appears in roughly the same direction from Earth as the Sun (the greatest elongation is 47.8°), so on Earth it can usually only be seen a few hours before sunrise or a few hours after sunset. However, when at its brightest, Venus may be seen during the daytime, making it one of only two heavenly bodies that can be seen both day and night (the other being the Moon). It is sometimes referred to as the "Morning Star" or the "Evening Star", and when it is visible in dark skies it is by far the brightest star-like object in the sky.

The cycle between one maximum elongation and the next lasts 584 days. After these 584 days Venus is visible in a position 72 degrees away from the previous one. Since 5 * 584 = 2920, which is equivalent to 8 * 365 Venus returns to the same point in the sky every 8 years (minus two leap days). This was known as the Sothis cycle in ancient Egypt, and was familiar to the Maya as well. Another association is with the Moon, because 2920 days equal almost exactly 99 lunations (29.5 * 99 = 2920.5).

Venus has a very slow retrograde rotation, meaning that, unlike with most planets, the direction of rotation on its axis is the opposite of its orbital revolution around the Sun. The very slow rotation means that the distinction between its Sidereal day (rotation relative to the stars) and Solar day (relative to the Sun) is very significant.

The pentagram has long been associated with the planet Venus and the worship of the goddess Venus, or her equivalent. It is most likely to have originated from the observations of prehistoric astronomers. When viewed from Earth, the successive conjunctions of Venus plot the points of a pentagram around the Sun every eight years, returning to its starting point after a forty year cycle.

Venus was known to ancient Babylonians around 1600 BC, and to the Mayan civilization (the Mayans developed a religious calendar based on Venus's motion) and must have been known long before in prehistoric times, given that it is the third brightest object in the sky after the Sun and Moon. The Maasai people in Africa named the planet Kileken, and have a myth about it called "The Orphan Boy." The Morning Star was called the Bearer of Light ("phōsphoros" or "eōsphoros" in Greek and "Lucifer" in Latin, a term later used of the fallen angel cast out of heaven, see Isaiah 14:12). To the Jews it was known as Noga ("shining") and it was used in rabbinic literature as a symbol of beauty and purity

♀

Its symbol is the sign also used in biology for the female sex, a stylized representation of the goddess Venus's hand mirror: a circle with a small cross underneath (Unicode: ♀). The Venus symbol also represents femininity, and in ancient alchemy stood for copper. Alchemists constructed the symbol from a circle (representing spirit) above a cross (representing matter).

The association with sex and femininity is supposed to relate to the period of 266 days between the conjunction and maximum elongation of Venus, which corresponds more or less to the length of human pregnancy.

The adjective Venusian is commonly used for Venus, but it is etymologically incorrect. The true adjective coming from Latin, Venereal, is avoided because of its modern association with sexually transmitted diseases. Some astronomers use Cytherean, which comes from Cythera. Other less common adjectives include Venerean, Venerian, and Veneran.

The Chinese, Korean, Japanese and Vietnamese cultures refer to the planet as the metal star, 金星, based on the Five Elements.

Contents

Physical characteristics

Atmosphere

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 oceans); its atmosphere is also roughly 90 times more massive than ours. This enormously CO2-rich atmosphere results in a strong greenhouse effect that raises the surface temperature more than 400 °C (750 °F) above what it would be otherwise, causing temperatures at the surface to reach extremes as great as 500 °C (930 °F) in low elevation regions near the planet's equator. This makes Venus's surface hotter than Mercury's, even though Venus is nearly twice as distant from the Sun and only receives 25% of the solar irradiance (2613.9 W/m² in the upper atmosphere, and just 1071.1 W/m² at the surface). Owing 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 of less than one rotation per Venusian year, meaning that, at the equator, Venus' surface rotates at a mere 6.5 km/h (4 mph). Upper atmosphere winds circling the planet approximately every 4 days help distribute the heat to other areas on the surface.

The solar irradiance is so much lower at the surface of Venus because the planet's thick cloud cover reflects the majority of the sunlight back into space. This prevents most of the sunlight from ever heating the surface. Venus's bolometric albedo is approximately 60%, and its visual light albedo is even greater. Thus, despite being closer to the Sun than Earth, the surface of Venus is not as well heated and even less well lit by the Sun. In the absence of any greenhouse effect, the temperature at the surface of Venus would be quite similar to Earth. A common conceptual misunderstanding regarding Venus is the mistaken belief that its thick cloud cover traps heat, as the opposite is actually true. The cloud cover keeps the planet much cooler than it would be otherwise. The immense quantity of CO2 in the atmosphere is what traps the heat by the greenhouse mechanism.

There are strong 300 km/h (200 mph) winds at the cloud tops, but winds at the surface are very slow, no more than a few miles per hour. However, owing 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 mainly composed of sulfur dioxide and sulfuric acid droplets and cover the planet completely, obscuring any surface details from the human eye. The temperature at the tops of these clouds is approximately −45 °C (−50 °F). The mean surface temperature of Venus, as given by NASA, is 464 °C (864 °F). The minimal value of the temperature, listed in the table, refers to cloud tops —the surface temperature is never below 400 °C (750 °F). (This makes the surface temperature hot enough to melt lead.)

The atmosphere also contains hydrogen sulfide (H2S) and carbonyl sulfide (SCO). Hydrogen sulfide reacts with sulfur dioxide, which implies that some process must be creating these components. It is unclear how the carbonyl sulfide could be formed--it is often a sign of biological activity. Some have suggested that microbes exist in the clouds (which also contain droplets of water), and produce these components from water, carbon monoxide and sulfur dioxide. New Scientist, Sept. 28, 2002, p. 16

Surface features

Radar image of the surface of Venus, centered at 180 degrees east longitude.
Enlarge
Radar image of the surface of Venus, centered at 180 degrees east longitude.
For more details on this topic, see Geology of Venus.

Venus has slow retrograde rotation, meaning it rotates from east to west, instead of west to east as most of the other major planets do. (Pluto and Uranus also have retrograde rotation, though Uranus's axis, tilted at 97.86 degrees, almost lies in its orbital plane.) It is not known 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. If the Sun could be seen from Venus' surface, it would appear to rise and set in a 116.75 day cycle (Venus' synodic rotation period), and a Venusian year would thus last 1.92 Venusian "days".

In addition to this unusual retrograde rotation, the periods of Venus' 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 simply be a coincidence, but there is some speculation that this may be the result of tidal locking, with tidal forces affecting Venus' rotation whenever the planets get close enough together —although the tides raised by Earth on Venus are vanishingly small.

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 2 km 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. Venus' thick atmosphere causes meteors to decelerate as they fall toward the surface, and even large meteors will strike the surface at too low a speed to form an impact crater if they have less than a certain threshold kinetic energy. Because of this, no impact crater smaller than about 3 km (2 mi) in diameter can form.

Nearly 90% of Venus's surface appears to consist of recently (in the geological sense) solidified basaltic lava, with very few meteorite craters. 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). This suggests that Venus underwent a major resurfacing event in the not too distant geological past. The interior of Venus is probably 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 as Earth does, but instead undergoes massive volcanic upwellings at regular intervals that inundate its surface with fresh lava. Other recent findings suggest that Venus is still volcanically active in isolated geological hotspots.

Venus's intrinsic magnetic field has been found very weak compared to other planets in the solar system. This may be due to its slow rotation being insufficient to drive an internal dynamo of liquid iron. As a result, solar wind strikes Venus's upper atmosphere without mediation. 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 owing 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. Molecular oxygen is thought to have combined with atoms in the crust (large amounts of oxygen, however, remain in the atmosphere in the form of carbon dioxide). Because of their dryness, Venus's rocks are much harder than Earth's, which leads to steeper mountains, cliffs and other features.

Venus' moon

Venus was once thought to possess a moon, named Neith after the chief goddess of Sais, Egypt (whose veil no mortal raised), first observed by Giovanni Domenico Cassini in 1672. German astronomers called the moon Kleinchen (literally "tiny"), and sporadic sightings by astronomers continued until 1892. These sightings have since been discredited, and are thought to have been either spurious internal reflections, mostly faint stars that happened to be in the right place at the right time, or maybe even asteroids passing by the planet. Venus is now known to be moonless.

Observations and explorations of Venus

Main article: Observations and explorations of Venus

Venus has been observed several times within the past 4000 years by a number of people, including the Greeks.

Appearance

Greatest Eastern Elongation Maximum brightness Stationary, begin retrograde Inferior Conjunction Stationary, resume direct Maximum brightness Greatest Western Elongation Superior Conjunction
March 29, 2004 46° May 3, 2004 May 18, 2004 June 8, 2004 June 29, 2004 July 13, 2004 August 17, 2004 45.8° March 31, 2005
November 3, 2005 47.1° December 12, 2005 December 23, 2005 January 13, 2006 February 3, 2006 February 14, 2006 March 25, 2006 46.5° October 27, 2006
June 9, 2007 45.4° July 14, 2007 July 25, 2007 August 18, 2007 September 7, 2007 September 23, 2007 October 28, 2007 46.5° June 9, 2008
January 14, 2009 47.1° February 20, 2009 March 5, 2009 March 27, 2009 April 15, 2009 April 29, 2009 June 5, 2009 45.9° January 11, 2010
August 20, 2010 46° September 27, 2010 October 7, 2010 October 29, 2009 November 16, 2010 December 2, 2010 January 8, 2011 47° August 16, 2011
March 27, 2012 46° April 30, 2012 May 15, 2012 June 6, 2012 June 27, 2012 July 10, 2012 August 15, 2012 45.8° March 28, 2013
November 1, 2013 47.1° December 10, 2013 December 20, 2013 January 11, 2014 January 31, 2014 February 11, 2014 March 22, 2014 46.6° October 25, 2014
June 6, 2015 45.4° July 12, 2015 July 23, 2015 August 15, 2015 September 5, 2015 September 20, 2015 October 26, 2015 46.4° June 6, 2016
January 12, 2017 47.1° February 18, 2017 March 2, 2017 March 25, 2017 April 12, 2017 April 26, 2017 June 3, 2017 45.9° January 9, 2018
August 17, 2018 45.9° September 25, 2018 October 5, 2018 October 26, 2018 November 24, 2018 November 30, 2018 January 6, 2019 47° August 14, 2019
March 24, 2020 46.1° April 28, 2020 May 13, 2020 June 3, 2020 June 24, 2020 July 8, 2020 August 13, 2020 45.8° March 26, 2021

Lowest distances to earth

At inferior conjunction, Venus can get closer to earth than any other planet--little more than 100 times the Moon's average distance. On December 16th, 1850, Venus reached since 1800 the lowest distance to earth with a value of 0,264138541298281 AU = 39514827 kilometres. This will be the closest approach of Venus to earth since December 16th, 2101 when Venus will reach a distance of 0,26431736 AU = 39541578 kilometres to earth.

Cultural references

See also Venus in fiction

Until it was penetrated by probes, Venus's opaque cloud layer gave science fiction writers free rein in imagining the planet's surface, and they frequently imagined it to be Earthlike. There are some religious sects who believe that Hell may be located on Venus. Its extremely high surface temperature and impenetrable cloud cover cause people to believe that the fires of Hell burn on the surface, obscured from our earthly view. Conversely, other sects consider Venus to be some form of paradise or an advanced secret base for angels/aliens to operate from.

  • In Olaf Stapledon's epic Last and First Men (1930), Venus is an oceanic idyll where humans evolve the power of flight.
  • In the mythology of Middle-earth (1937), by J. R. R. Tolkien, Venus is the Star of Eärendil. The star was created when Eärendil the Mariner was set in the sky on his ship, with a Silmaril bound to his brow. In fact, Tolkien chose the name directly from the ancient Old English word for the planet Venus.
  • In H. P. Lovecraft's Cthulhu Mythos (1928–), there are mentions of the 'Lords of Venus', and conflicting indications that the Serpent People originated there.
  • Edgar Rice Burroughs wrote a series of five books on Venus, featuring hero Carson Napier, who discovers that Venus (or Amtor, as it is known by the Venusians) is a world of sky-high trees, warring kingdoms and princesses in need of rescue. [1]
  • The H. P. Lovecraft and Kenneth Sterling short story 'In the Walls of Eryx' (1939), takes place on Venus, but is not considered part of the Cthulhu Mythos.
  • The second book of the Space Trilogy (19381945) by C.S. Lewis, Perelandra 1943) takes place on Venus (called by the natives Perelandra), the site of a second garden of Eden.
  • In the military science fiction classic Clash by Night (1943) by Henry Kuttner (writing as Lawrence O'Donnell) and C. L. Moore, underwater city-states hire mercenary companies and their battleships to fight their wars on the surface.
  • Venus was the home planet of the Mekon, arch-enemy of the 1950s comic book hero Dan Dare.
  • Many science-fiction movies and serials of the '50s and '60s, such as Abbott and Costello Go to Mars and Space Patrol, have used Venus' namesake goddess and her domain to contrive planetary populations of nubile women welcoming (or attacking) all-male astronaut crews.
  • In the Noon Universe created by the Soviet science fiction writers Boris and Arkady Strugatsky, Venus is depicted as a extremely harsh planet covered by strange flora and fauna but also very rich in minerals and heavy metals. The novel The Land of Crimson Clouds (Strana Bagrovykh Tuch in the original) describes the first successful manned mission to Venus, although a full-scaled colonization of the planet was not initiated until much later (in 2119; see Noon: 22nd Century).
  • Venus is the location of several Starfleet Academy training facilities and terraforming stations in the fictional Star Trek universe (1966–).
  • In Jacqueline Susann's Yargo (1979), Venus is inhabited by bees that are as big as horses.
  • Venus is briefly mentioned in Arthur C. Clarke's 3001: The Final Odyssey (1997).
  • A presumably terraformed Venus was the setting of one episode of the anime Cowboy Bebop (1998). In the show, Venus was revealed to be an arid but habitable world. Much of the population lived in floating cities in the sky. In the cartoon Exosquad, terraformed Venus was portrayed as one of the three habitable planets in the solar system (the others being Earth and Mars).
  • In the Japanese anime series, Bishoujo Senshi Sailor Moon (1992), Sailor Venus is a soldier representing the planet of the same name. In mythology, Venus is the Roman goddess of love (Aphrodite in Greek), therefore, Sailor Venus's attacks and weapons (e.g. Venus Love Me Chain and Venus Love and Beauty Shock) represent the idea of love and femininity. Her image colours are gold and orange--similar to the colour of the planet. Also, on her forehead is the planet's symbol.
  • A more scientifically accurate depiction of the planet is offered in Ben Bova's novel Venus (2000, ISBN 031287216X)-

See also

Commons
Wikimedia Commons has media related to:

References

Pentagram


The Solar System
Sun - Mercury - Venus - Earth (Moon) - Mars - Asteroid belt - Jupiter
Saturn - Uranus - Neptune - Pluto - Kuiper belt - Scattered disc - Oort cloud
See also astronomical objects and the solar system's list of objects, sorted by radius or mass.

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