About: Reiden Patera

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Reiden Patera is a volcanic feature on Jupiter's moon Io. It was first detected by the Galileo SSI Team during the spacecraft Galileo's first orbit around Jupiter, initially detected as a hotspot. It was once thought that the activity there had stopped or waned below the limits of the spacecraft's Solid State Imager or Near-Infrared Mapping Spectrometer. However, it was noticed in 2002 that Reiden Patera has darkened considerably since the 24th orbit of Galileo. It has been spouting bright red pyroclastic deposits of its own. It is located at 13°24′S 235°27′W / 13.4°S 235.45°W and is 70 kilometers in diameter. It is named after a Japanese thunder god ("Raijin" in current English nomenclature). Asha Patera can be found to the east, and Kami-Nari Patera can be found to the north.

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  • Reiden Patera is a volcanic feature on Jupiter's moon Io. It was first detected by the Galileo SSI Team during the spacecraft Galileo's first orbit around Jupiter, initially detected as a hotspot. It was once thought that the activity there had stopped or waned below the limits of the spacecraft's Solid State Imager or Near-Infrared Mapping Spectrometer. However, it was noticed in 2002 that Reiden Patera has darkened considerably since the 24th orbit of Galileo. It has been spouting bright red pyroclastic deposits of its own. It is located at 13°24′S 235°27′W / 13.4°S 235.45°W and is 70 kilometers in diameter. It is named after a Japanese thunder god ("Raijin" in current English nomenclature). Asha Patera can be found to the east, and Kami-Nari Patera can be found to the north. (en)
  • Reiden Patera est une caractéristique volcanique sur Io, un satellite naturel de Jupiter. Elle est détectée pour la première fois par l'équipe Galileo SSI en 1996 lors de la première orbite de la sonde spatiale autour de Jupiter, initialement supposée comme étant un point chaud. Ensuite, l'activité observée diminue en dessous des limites de l'imageur à semi-conducteurs ou du spectromètre de cartographie proche infrarouge de la sonde. Cependant, en 2002, il est observé que Reiden Patera s'était considérablement assombrie depuis la 24ème orbite de Galileo. Il y jaillit des nuées ardentes rouge vif. Elle est située à 13°24′S 235°27′W / 13.4°S 235.45°W et possède un diamètre de 70 km. Elle porte le nom d'un dieu du tonnerre japonais Raiden. Asha Patera se trouve à l'est, et Kami-Nari Patera se trouve au nord. (fr)
  • La Reiden Patera è una struttura geologica della superficie di Io. (it)
  • ライデン火口(ライデンかこう)は、木星の衛星イオにある火山地形。探査機ガリレオのSSIチームが、ガリレオの木星を公転する最初の軌道で最初に検出され、最初はホットスポットだと思われた。当時は、そこの活動は止まっているか、探査機の固体撮像機や近赤外線分光器が検出できないほどにまで弱まっていると考えられた。しかし、2002年に、ガリレオの軌道の24周目以降、ライデン火口がかなり暗くなっていることが発見された。ライデン火口は明るい赤色の火砕流を放出し続けていたのである。ライデン火口は南緯13度24分 西経235度27分 / 南緯13.4度 西経235.45度にあり、直径は70 kmである。ライデン火口の名は日本の雷神に由来する。東にが、北にはカミナリ火口がある。 (ja)
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  • Reiden Patera is a volcanic feature on Jupiter's moon Io. It was first detected by the Galileo SSI Team during the spacecraft Galileo's first orbit around Jupiter, initially detected as a hotspot. It was once thought that the activity there had stopped or waned below the limits of the spacecraft's Solid State Imager or Near-Infrared Mapping Spectrometer. However, it was noticed in 2002 that Reiden Patera has darkened considerably since the 24th orbit of Galileo. It has been spouting bright red pyroclastic deposits of its own. It is located at 13°24′S 235°27′W / 13.4°S 235.45°W and is 70 kilometers in diameter. It is named after a Japanese thunder god ("Raijin" in current English nomenclature). Asha Patera can be found to the east, and Kami-Nari Patera can be found to the north. (en)
  • La Reiden Patera è una struttura geologica della superficie di Io. (it)
  • ライデン火口(ライデンかこう)は、木星の衛星イオにある火山地形。探査機ガリレオのSSIチームが、ガリレオの木星を公転する最初の軌道で最初に検出され、最初はホットスポットだと思われた。当時は、そこの活動は止まっているか、探査機の固体撮像機や近赤外線分光器が検出できないほどにまで弱まっていると考えられた。しかし、2002年に、ガリレオの軌道の24周目以降、ライデン火口がかなり暗くなっていることが発見された。ライデン火口は明るい赤色の火砕流を放出し続けていたのである。ライデン火口は南緯13度24分 西経235度27分 / 南緯13.4度 西経235.45度にあり、直径は70 kmである。ライデン火口の名は日本の雷神に由来する。東にが、北にはカミナリ火口がある。 (ja)
  • Reiden Patera est une caractéristique volcanique sur Io, un satellite naturel de Jupiter. Elle est détectée pour la première fois par l'équipe Galileo SSI en 1996 lors de la première orbite de la sonde spatiale autour de Jupiter, initialement supposée comme étant un point chaud. Ensuite, l'activité observée diminue en dessous des limites de l'imageur à semi-conducteurs ou du spectromètre de cartographie proche infrarouge de la sonde. Cependant, en 2002, il est observé que Reiden Patera s'était considérablement assombrie depuis la 24ème orbite de Galileo. Il y jaillit des nuées ardentes rouge vif. (fr)
rdfs:label
  • Reiden Patera (fr)
  • Reiden Patera (it)
  • ライデン火口 (ja)
  • Reiden Patera (en)
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