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Angustus Labyrinthus is a complex of intersecting valleys or ridges near the Martian south pole (in the Mare Australe quadrangle), located at 81.68° S and 63.25° W. It was nicknamed the "Inca City" by NASA scientists due to its superficial resemblance to a ruined city. Like other formations in the area, the name 'Angustus' derives from a name given by Eugene Antoniadi in 1930 to an albedo feature that corresponds with the area. The name was approved in 2006.

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  • Angustus Labyrinthus (en)
  • Angustus Labyrinthus (ca)
  • Angustus Labyrinthus (it)
  • Angustus Labyrinthus (pt)
  • 安古斯都迷宫 (zh)
rdfs:comment
  • Angustus Labyrinthus és una formació geològica de tipus labyrinthus a la superfície de Mart, localitzada amb el sistema de coordenades planetocèntriques a -81.16 ° latitud N i 298.59 ° longitud E, que fa 67.52 km de diàmetre. El nom va ser aprovat per la UAI el 13 de setembre de 2006 i fa referència a una característica d'albedo. (ca)
  • L'Angustus Labyrinthus (latino per "Labirinto angusto") è una formazione geologica della superficie di Marte, posta in prossimità del polo sud del pianeta. Il nome, approvato dall'Unione astronomica internazionale nel 2006, deriva da quello attribuito nel 1930 da Eugène Antoniadi a una caratteristica di albedo corrispondente a quest'area. (it)
  • Angustus Labyrinthus é um complexo de várias interseções de vales e tergos no quadrângulo de Mare Australe, localizado a 81.68º S e 63.25º W. Essa região possui 75 km de uma ponta a outra e recebeu um nome clássico para uma formação de albedo. (pt)
  • 安古斯都迷宫(Angustus Labyrinthus)是火星南海区位于南纬81.68度和西经63.25度附近一处河谷或山脊交错的区域。由于表面类似于一座废墟,美国宇航局科学家们将它戏称为“印加城”。与该地区的其他构造一样,“安古斯都”一词源于1930年欧仁·安东尼亚第对该地区反照率特征的命名。2006年,该名称被国际天文联合会正式采用。 安古斯都迷宫是由水手9号探测器所发现,它拍摄到一处看上去像一座古城废墟的小区域。水手9号研究团队将其命名为“印加城”。它看起来就像由两种不同风向形成的沙丘,但只是这些过于沙丘巨大。2002年,火星全球探勘者号上的相机发现,“印加城”是一座直径86公里大型圆形结构的一部分,因此,该形状意味着它可能是由小行星撞击造成,小行星撞击使地壳破裂。后来,岩浆沿着裂缝流动,在冷却后,形成坚硬、耐侵蚀的岩壁(岩脉)。陨石坑被覆盖,然后又被部分挖掘暴露。随着周围较松软材料的侵蚀,坚硬的岩壁被保留了下来。 (zh)
  • Angustus Labyrinthus is a complex of intersecting valleys or ridges near the Martian south pole (in the Mare Australe quadrangle), located at 81.68° S and 63.25° W. It was nicknamed the "Inca City" by NASA scientists due to its superficial resemblance to a ruined city. Like other formations in the area, the name 'Angustus' derives from a name given by Eugene Antoniadi in 1930 to an albedo feature that corresponds with the area. The name was approved in 2006. (en)
name
  • Angustus Labyrinthus (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Angustus_Labyrinthus.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Inca_City.jpg
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  • Angustus Labyrinthus, as seen by THEMIS. (en)
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  • -81.68 -63.25
has abstract
  • Angustus Labyrinthus és una formació geològica de tipus labyrinthus a la superfície de Mart, localitzada amb el sistema de coordenades planetocèntriques a -81.16 ° latitud N i 298.59 ° longitud E, que fa 67.52 km de diàmetre. El nom va ser aprovat per la UAI el 13 de setembre de 2006 i fa referència a una característica d'albedo. (ca)
  • Angustus Labyrinthus is a complex of intersecting valleys or ridges near the Martian south pole (in the Mare Australe quadrangle), located at 81.68° S and 63.25° W. It was nicknamed the "Inca City" by NASA scientists due to its superficial resemblance to a ruined city. Like other formations in the area, the name 'Angustus' derives from a name given by Eugene Antoniadi in 1930 to an albedo feature that corresponds with the area. The name was approved in 2006. Angustus Labyrinthus was discovered by the Mariner 9 probe, which photographed a small area that looked like the ruins of an ancient city. Mariner 9 team members named it the "Inca City". It looked like sand dunes that had formed from winds that blew from two different directions, but the dunes were too big. In 2002 the camera on Mars Global Surveyor revealed that the 'Inca City' was part of a large circular structure that was 86 km in diameter. So the shape meant that it was probably caused by an asteroid impact which cracked the crust. Later, magma flowed along the cracks. When the magma cooled, hard, erosion resistant walls of rock (dikes) formed. The crater was covered over, then partially exhumed. The hard walls of rock were left standing as softer surrounding material eroded away. (en)
  • L'Angustus Labyrinthus (latino per "Labirinto angusto") è una formazione geologica della superficie di Marte, posta in prossimità del polo sud del pianeta. Il nome, approvato dall'Unione astronomica internazionale nel 2006, deriva da quello attribuito nel 1930 da Eugène Antoniadi a una caratteristica di albedo corrispondente a quest'area. (it)
  • Angustus Labyrinthus é um complexo de várias interseções de vales e tergos no quadrângulo de Mare Australe, localizado a 81.68º S e 63.25º W. Essa região possui 75 km de uma ponta a outra e recebeu um nome clássico para uma formação de albedo. (pt)
  • 安古斯都迷宫(Angustus Labyrinthus)是火星南海区位于南纬81.68度和西经63.25度附近一处河谷或山脊交错的区域。由于表面类似于一座废墟,美国宇航局科学家们将它戏称为“印加城”。与该地区的其他构造一样,“安古斯都”一词源于1930年欧仁·安东尼亚第对该地区反照率特征的命名。2006年,该名称被国际天文联合会正式采用。 安古斯都迷宫是由水手9号探测器所发现,它拍摄到一处看上去像一座古城废墟的小区域。水手9号研究团队将其命名为“印加城”。它看起来就像由两种不同风向形成的沙丘,但只是这些过于沙丘巨大。2002年,火星全球探勘者号上的相机发现,“印加城”是一座直径86公里大型圆形结构的一部分,因此,该形状意味着它可能是由小行星撞击造成,小行星撞击使地壳破裂。后来,岩浆沿着裂缝流动,在冷却后,形成坚硬、耐侵蚀的岩壁(岩脉)。陨石坑被覆盖,然后又被部分挖掘暴露。随着周围较松软材料的侵蚀,坚硬的岩壁被保留了下来。 (zh)
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  • POINT(-63.25 -81.680000305176)
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