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Phoebe Regio
Phoebe Regio is a regio on the planet Venus. It lies to the southeast of Asteria Regio. It is in diameter and is the principal feature of the V41 quadrangle, to which it gave its name. Four Soviet landers, Venera 11, Venera 12, Venera 13 and Venera 14 Venera 14 (russian: Венера-14 meaning Venus 14) was a probe in the Soviet Venera program for the exploration of Venus. Venera 14 was identical to the Venera 13 spacecraft, built to take advantage of the 1981 Venus launch opportunity. Vene ..., landed on the eastern side of Phoebe Regio and performed various scientific measurements. References Surface features of Venus {{crater-stub ...
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Asteria And Phoebe Regio
Asteria may refer to: *Asteria (mythology), any one of various female figures in Greek mythology *Asteria (band), an American band *ASTERIA (spacecraft), a miniaturized space telescope *Asteria Regio, a region on the planet Venus *Asteria Medievale, a medieval music ensemble See also *''Asterias'', a genus of sea star *Asterism (gemology) An asterism () is a star-shaped concentration of reflected or refracted light from a gemstone. Asterisms can appear when a suitable stone is cut ''en cabochon'' i.e. shaped and polished (not faceted). A gemstone that exhibits this effect is re ...
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Asteria Regio
Asteria Regio is a region on the planet Venus. It is bordered on the southeast by Phoebe Regio. It is located in the Hecate Chasma Hecate or Hekate, , ; grc-dor, Ἑκάτᾱ, Hekátā, ; la, Hecatē or . is a goddess in ancient Greek religion and mythology, most often shown holding a pair of torches, a key, snakes, or accompanied by dogs, and in later periods depict ... (v28) quadrangle. References Guinevere Planitia quadrangle Surface features of Venus {{crater-stub ...
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Magellan (spacecraft)
The ''Magellan'' spacecraft was a robotic space probe launched by NASA of the United States, on May 4, 1989, to map the surface of Venus by using synthetic-aperture radar and to measure the planetary gravitational field. The ''Magellan'' probe was the first interplanetary mission to be launched from the Space Shuttle, the first one to use the Inertial Upper Stage booster, and the first spacecraft to test aerobraking as a method for circularizing its orbit. ''Magellan'' was the fifth successful NASA mission to Venus, and it ended an eleven-year gap in U.S. interplanetary probe launches. History Beginning in the late 1970s, scientists advocated for a radar mapping mission to Venus. They first sought to construct a spacecraft named the ''Venus Orbiting Imaging Radar'' (VOIR), but it became clear that the mission would be beyond the budget constraints during the ensuing years. The VOIR mission was canceled in 1982. A simplified radar mission proposal was recommended by the Solar ...
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Phoebe (mythology)
In ancient Greek religion and mythology, Phoebe ( ; grc, Φοίβη, Phoíbē, associated with ''phoîbos'', "shining") was one of the first generation of Titans, who were one set of sons and daughters of Uranus and Gaia.Hesiod, ''Theogony'116-138 She was the grandmother of the sun god Apollo, the moon goddess Artemis, and the witchcraft goddess Hecate. According to myth, she was the original owner of the Oracle of Delphi before gifting it to her grandson Apollo. Her name, meaning "bright", was also given to a number of lunar goddesses like Artemis and later the Roman goddesses Luna and Diana, but Phoebe herself was not actively treated as a moon goddess on her own right in ancient mythology. Etymology Greek , feminine form of ' means "pure, bright".'' A Greek-English Lexicon'' s.vφοῖβος Another meaning is "prophet", a reference to her role in myth. Used for water and fire both, it can thus be explained as generally meaning "pure", "clear", or "bright". Family Pho ...
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Planetary Geology
Planetary geology, alternatively known as astrogeology or exogeology, is a planetary science discipline concerned with the geology of the celestial bodies such as the planets and their moons, asteroids, comets, and meteorites. Although the geo- prefix typically indicates topics of or relating to Earth, planetary geology is named as such for historical and convenience reasons; due to the types of investigations involved, it is closely linked with Earth-based geology. These investigations are centered around the composition, structure, processes, and history of a planet. Planetary geology includes such topics as determining the properties and processes of the internal structure of the terrestrial planets, and also looks at planetary volcanism and surface processes such as impact craters, fluvial and aeolian processes. The structures and compositions of the giant planets and their moons are also examined, as is the make-up of the minor bodies of the Solar System, such as aster ...
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Venus
Venus is the second planet from the Sun. It is sometimes called Earth's "sister" or "twin" planet as it is almost as large and has a similar composition. As an interior planet to Earth, Venus (like Mercury) appears in Earth's sky never far from the Sun, either as morning star or evening star. Aside from the Sun and Moon, Venus is the brightest natural object in Earth's sky, capable of casting visible shadows on Earth at dark conditions and being visible to the naked eye in broad daylight. Venus is the second largest terrestrial object of the Solar System. It has a surface gravity slightly lower than on Earth and has a very weak induced magnetosphere. The atmosphere of Venus, mainly consists of carbon dioxide, and is the densest and hottest of the four terrestrial planets at the surface. With an atmospheric pressure at the planet's surface of about 92 times the sea level pressure of Earth and a mean temperature of , the carbon dioxide gas at Venus's surface is in the ...
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List Of Quadrangles On Venus
The surface of Venus has been divided into 8 quadrangles at the 1:10,000,000 map scale, or 62 quadrangles at the 1:5,000,000 map scale. 1:10,000,000 map scale 1:5,000,000 map scale See also * List of quadrangles on Mercury * List of quadrangles on the Moon * List of quadrangles on Mars The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. Each quadrangle is a region covering a specified range of latitudes and longitudes on the Martian surface. The quadrangles are name ... References {{DEFAULTSORT:Quadrangles on Venus * Venus-related lists ...
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United States Geological Survey
The United States Geological Survey (USGS), formerly simply known as the Geological Survey, is a scientific agency of the United States government. The scientists of the USGS study the landscape of the United States, its natural resources, and the natural hazards that threaten it. The organization's work spans the disciplines of biology, geography, geology, and hydrology. The USGS is a fact-finding research organization with no regulatory responsibility. The agency was founded on March 3, 1879. The USGS is a bureau of the United States Department of the Interior; it is that department's sole scientific agency. The USGS employs approximately 8,670 people and is headquartered in Reston, Virginia. The USGS also has major offices near Lakewood, Colorado, at the Denver Federal Center, and Menlo Park, California. The current motto of the USGS, in use since August 1997, is "science for a changing world". The agency's previous slogan, adopted on the occasion of its hundredt ...
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Venera 11
The Venera 11 (russian: Венера-11 meaning ''Venus 11'') was a Soviet uncrewed space mission which was part of the Venera program to explore the planet Venus. Venera 11 was launched on 9 September 1978 at 03:25:39 UTC. Separating from its flight platform on December 23, 1978 the lander entered the Venus atmosphere two days later on December 25 at 11.2 km/s. During the descent, it employed aerodynamic braking followed by parachute braking and ending with atmospheric braking. It made a soft landing on the surface at 06:24 Moscow Time (03:24 UT) on 25 December after a descent time of approximately 1 hour. The touchdown speed was 7 to 8 m/s. Information was transmitted to the flight platform for retransmittal to earth until it moved out of range 95 minutes after touchdown. Landing coordinates are . Flight platform After ejection of the lander probe, the flight platform continued on past Venus in a heliocentric orbit. Near encounter with Venus occurred on December 2 ...
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Venera 12
The Venera 12 (russian: Венера-12 meaning Venus 12) was an uncrewed Soviet space mission designed to explore the planet Venus. Venera 12 was launched on 14 September 1978 at 02:25:13 UTC. After separating from its flight platform on 19 December 1978, the Venera 12 lander entered the Venus atmosphere two days later at 11.2 km/s. During its descent, the lander employed aerodynamic braking followed by parachute braking, ending with atmospheric braking. After a nearly one-hour descent, a soft landing was made at 06:30 Moscow time (0330 UT) on 21 December. Touchdown speed was 7–8 m/s; landing coordinates are . Continuing for about 110 minutes after touchdown, the lander transmitted data to the flight platform for about 110 minutes until the flight platform, which remained in a heliocentric orbit, moved out of range. Venera 11 and 12 carried identical instruments. Flight platform The Venera 12 flight platform carried solar wind detectors, ionosphere electron instr ...
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Venera 13
Venera 13 (russian: Венера-13 meaning Venus 13) was part of the Soviet Venera program meant to explore Venus. Venera 13 and 14 were identical spacecraft built to take advantage of the 1981 Venus launch opportunity. The probes were launched five days apart, with Venera 13 launching on 30 October 1981 at 06:04 UTC and Venera 14 launching on 4 November 1981 at 05:31 UTC. Both had an on-orbit dry mass of 760 kg. Venera 13 transmitted the first recording of actual sounds from another planet, including sounds of Venusian wind, the lander hitting the ground, pyrotechnic lens cap removal and its impact on regolith, and action of the regolith drilling apparatus. Design The descent lasted about an hour. Venera 13 landed at 03:57:21 UT at 7.5 S, 303 E, just east of the eastern extension of an elevated region known as Phoebe Regio. The area is composed of bedrock outcrops surrounded by dark, fine-grained soil. Cruise stage As the cruise stage flew by Venus, the bus acted as a da ...
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Venera 14
Venera 14 (russian: Венера-14 meaning Venus 14) was a probe in the Soviet Venera program for the exploration of Venus. Venera 14 was identical to the Venera 13 spacecraft, built to take advantage of the 1981 Venus launch opportunity. Venera 14 was launched on 4 November 1981 at 05:31:00 UTC, five days after Venera 13 launched on 30 October 1981 at 06:04:00 UTC. Both had an on-orbit dry mass of . Design Each mission consisted of a cruise stage and an attached descent craft. Cruise stage As the cruise stage flew by Venus, the bus acted as a data relay for the lander before continuing on to a heliocentric orbit. Venera 14 was equipped with a gamma-ray spectrometer, UV grating monochromator, electron and proton spectrometers, gamma-ray burst detectors, solar wind plasma detectors, and two-frequency transmitters which made measurements before, during, and after the Venus flyby. Descent lander The descent lander was a hermetically sealed pressure vessel that contained most of ...
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