Fuchi Patera

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Fuchi Patera, in a screenshot taken in NASA World Wind. Click to enlarge. Amaterasu Patera.png
Fuchi Patera, in a screenshot taken in NASA World Wind. Click to enlarge.

Fuchi Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is approximately 66 kilometers in diameter and is located at 28°24′N327°36′W / 28.4°N 327.6°W / 28.4; -327.6 (Fuchi Patera) . It is named after the Ainu fire goddess, Kamuy Fuchi. Its name was adopted by the International Astronomical Union in 1979. [1] Manua Patera is located north-northeast, and Amaterasu Patera is located northeast. [2]

Patera (planetary nomenclature) irregular crater

Patera is an irregular crater, or a complex crater with scalloped edges on a celestial body. Paterae can have any origin, although majority of them were created by volcanism. The term comes from Latin language, where it refers to a shallow bowl used in antique culture.

Jupiter Fifth planet from the Sun in the Solar System

Jupiter is the fifth planet from the Sun and the largest in the Solar System. It is a giant planet with a mass one-thousandth that of the Sun, but two-and-a-half times that of all the other planets in the Solar System combined. Jupiter and Saturn are gas giants; the other two giant planets, Uranus and Neptune, are ice giants. Jupiter has been known to astronomers since antiquity. It is named after the Roman god Jupiter. When viewed from Earth, Jupiter can reach an apparent magnitude of −2.94, bright enough for its reflected light to cast shadows, and making it on average the third-brightest natural object in the night sky after the Moon and Venus.

Io (moon) Innermost of the four Galilean moons of Jupiter

Io is the innermost of the four Galilean moons of the planet Jupiter. It is the fourth-largest moon, has the highest density of all the moons, and has the least amount of water of any known astronomical object in the Solar System. It was discovered in 1610 and was named after the mythological character Io, a priestess of Hera who became one of Zeus' lovers.

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Reiden Patera patera on Io

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Amaterasu Patera patera on Io

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Asha Patera patera on Io

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Kami-Nari Patera patera on Io

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Manua Patera patera on Io

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Kinich Ahau Patera patera on Io

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Monan Patera patera on Io

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Ah Peku Patera patera on Io

Ah Peku Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is 84 kilometers in diameter and is located at 10.3°N 107°W. It is named after the Mayan thunder god Ah Peku. Its name was adopted by the International Astronomical Union in 2006. Ah Peku Patera is located on the south end of Monan Mons, north of which is Monan Patera. The eruptive centers Amirani and Maui can be found northwest, as well as Maui Patera. Gish Bar Patera is located toward the northeast. Ah Peku Patera was first detected by the spacecraft Galileo's Solid State Imager and Near-Infrared Mapping Spectrometer. It is considered an active hot spot.

Gish Bar Patera A complex crater with scalloped edges, on Jupiters moon Io

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Estan Patera patera on Io

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Shango Patera patera on Io

Shango Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is about 90 kilometers in diameter and is located at 32.35°N 100.52°W. It is named after the Yoruba thunder god Shango. Its name was approved by the International Astronomical Union in 2000. It is located north of Skythia Mons. To the southwest is the eruptive center Amirani, and to the southeast are Gish Bar Patera, Gish Bar Mons, and Estan Patera.

Maui Patera patera on Io

Maui Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is about 38 kilometers in diameter and is located at 16.61°N 124.25°W. It is named after Māui, a Hawaiian demigod that sought fire from Mafuike. Its name was approved by the International Astronomical Union in 1979. It is located southwest of the eruptive center Maui, south of Euxine Mons, and southwest of the volcano Amirani. Due east are Monan Patera, Monan Mons, and Ah Peku Patera.

Babbar Patera patera on Io

Babbar Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is about 86 kilometers in diameter and is located at 39.8°S 272°W. It is named after a Sumerian sun god, and its name was approved by the International Astronomical Union in 1979. Some scarps near Babbar Patera may represent faults. Immediately south of Babbar Patera is the plateau Lyrcea Planum, and further south is Svarog Patera. To the east is the mountain Egypt Mons.

Svarog Patera patera on Io

Svarog Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is 124 kilometers in diameter and is located at 48.66°S 265.74°W. It is named after the Russian smith god Svarog. Its name was approved by the International Astronomical Union in 1979. North of Svarog Patera is Lyrcea Planum, north of which is Babbar Patera. To the south is Silpium Mons, and to the east is Hermes Mensa. To the southeast are Pyerun Patera and Epaphus Mensa. Svarog Patera is a Voyager spacecraft-detected hot spot.

Pyerun Patera patera on Io

Pyerun Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is about 52 kilometers in diameter and is located at 55.64°S 251.21°W. It is named after the Slavonic god of thunder, Pyerun. The name was adopted by the International Astronomical Union in 1985. West of Pyerun Patera is Mithra Patera, and to the east is the mesa Epaphus Mensa. To the northeast is Epaphus Mensa, and to the northwest are the mountain Silpium Mons and Svarog Patera.

Mithra Patera patera on Io

Mithra Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is about 34 kilometers in diameter and is located at 59.0°S 266.46°W. It is named after the Persian god of light, Mithra. Its name was adopted by the International Astronomical Union in 1985. To the north is Silpian Mons, and to the east is Pyerun Patera. Located southwest is Viracocha Patera.

Viracocha Patera patera on Io

Viracocha Patera is a patera, or a complex crater with scalloped edges, on Jupiter's moon Io. It is about 59 kilometers in diameter and is located at 61.77°S 280.09°W. It is named after the Quechua creator god Viracocha. The name was adopted by the International Astronomical Union in 1979. Viracocha Patera is a Voyager spacecraft-detected hot spot. To Viracocha Patera's east-northeast is Mithra Patera, and to the northeast is the mountain Silpium Mons.

Silpium Mons mountain on Io

Silpium Mons is a mountain on Jupiter's moon Io. It is 5.6 kilometers in height, 113 kilometers in length, and 79.7 kilometers in width. It covers an area of 7073 km2. It is a striated ridge, meaning it is an elevated structure dominated by one or more prominent linear or arcurate rises. It is named after a location in Greece where the mythological Io died of grief. Its name was adopted by the International Astronomical Union in 1979. It is located at 52.71°S 272.34°W, south of Svarog Patera, north of Mithra Patera, and northeast of Viracocha Patera. Its proximity to Svarog and Viracocha Paterae has been suggested to be evidence for a structural relationship between mountains and calderas on Io.

Nili Patera dune field

Nili Patera is a dune field on Mars. It is located on top of a lava bed, at the site of an ancient volcano, the Nili Patera caldera of Syrtis Major, near the Martian equator, and it is one of the most active dune fields of Mars. Its location coordinates on Mars are 8.7° N latitude, 67.3° E longitude. It is being actively studied by the HiRISE camera, on board the Mars Reconnaissance Orbiter, at the rate of one image every six weeks. The study of the movement of the dunes provides information regarding wind variation as a function of time and furthers the study of surface erosion characteristics of the Martian landscape. This information can then be used for the development and design of future Mars expeditions. The dunes of the Patera field are of the barchan type and their study by HiRISE was the first one to establish dune and ripple movement of a minimum of 1 metre on Mars. The Patera dune field, was also the first to be investigated using the COSI-Corr software, which was originally developed to analyse the movement of earthbound dunes. The research results from the evidence provided by the monitoring of the Nili Patera field, indicate sand fluxes of the order of several cubic metres per metre per year, similar to the flux observed at the sand dunes of Victoria Valley in Antarctica.

References

  1. "Fuchi Patera" . Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. NASA World Wind 1.4. NASA Ames Research Center, 2007.