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The exact location proposed for this landing is 22.16 N and 342.05 E. [4] The Mawrth Vallis region is well studied with more than 40 papers published in peer-reviewed publications. Near the Mawrth channel is a 200 meter high plateau with many exposed layers.
Ares Vallis was the landing site of NASA's Mars Pathfinder spacecraft, which studied a region of the valley near the border with Chryse in 1997. Ares Vallis is in the Oxia Palus quadrangle of Mars. It has been argued that Uzboi , Ladon , Margaritifer and Ares valles, although now separated by large craters, once comprised a single outflow ...
Valles (singular vallis) on Mars are similar to valleys on Earth. Some features that take this title may be better described as canyons or chasmata ; see List of Chasmata on Mars . Coordinates are given as planetocentric latitude with east longitude.
Valles Marineris (/ ˈ v æ l ɪ s m ær ɪ ˈ n ɛər ɪ s /; [1] Latin for Mariner Valleys, named after the Mariner 9 Mars orbiter of 1971–72 which discovered it) is a system of canyons that runs along the Martian surface east of the Tharsis region. [2]
Interactive image map of the global topography of Mars. Hover your mouse over the image to see the names of over 60 prominent geographic features, and click to link to them. Coloring of the base map indicates relative elevations , based on data from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor .
The Uzboi-Landon-Morava (ULM) outflow system is a long series of channels and depressions that may have carried water across a major part of Mars. It starts with channels that drain into the Argyre basin in the Argyre quadrangle.
[31] [32] [33] Nirgal Vallis is a tributary of Uzboi Vallis. Nirgal Vallis is believed to have formed by groundwater sapping, not by precipitation. Spectral analyses has found phyllosilicates (clays) that are iron-magnesium smectites. [34] [35] Some researchers believe these were formed by interaction with groundwater. Over a wide area, Al ...
The Tiu Valles / ˈ t iː uː ˈ v æ l iː z / are an outflow channel system in the Oxia Palus quadrangle of Mars, centered at 16.23° North and 34.86° West. [1]They are 1,720 km (1,070 mi) long and were named after the word for "Mars" in Old English (West Germanic).
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