Coordinates | 81°10′N 284°24′E / 81.17°N 284.4°E |
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Abalos Mensa is a wedge-shaped mound,[1] or mensa and one of the named features in the vicinity of Planum Boreum, the Martian North pole. It is named after one of the classical albedo features on Mars.[2] Its name was officially approved by IAU in 2006. It extends from latitude 80.21°N to 82.4°N and from longitude 279.34°E to 290.52°E (69.48°W – 80.66°W).[2] Its centre is located at latitude 81.17°N, longitude 284.4°E (75.6°W), and has a diameter of 129.18 km.[2]
Abalos Mensa is a convex formation of approximately 180 kilometer span, with a top-view shaped like a wedge,[3][1] and lies immediately to the south of the Rupes Tenuis scarp, approximately at 285ºE.[1] In the neighbourhood of Abalos Mensa is the beginning of the dune field of Abalos Undae which continues in a southwestward direction after it emerges from the western end of a narrow channel separating Rupes Tenuis from Abalos Mensa.[3] Crotone crater, located at 82.2ºN, 290.0ºE with a 6.4 km diameter, is situated at the channel separating the Rupes Tenuis scarp from Abalos Mensa.[3] West of Abalos Mensa, parallel to and south of the Rupes Tenuis scarp, runs a narrow, low-altitude plain, named Tenuis Mensa, which exhibits a southward slope.[4][5] The southern part of Abalos Mensa ends in a scarp called Abalos Scopuli.[6]