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The Mare Tyrrhenum quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. This quadrangle is also referred to as MC-22 (Mars Chart-22). [1] It contains parts of the regions Tyrrhena Terra, Hesperia Planum, and Terra Cimmeria.
The Mare Australe quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Mare Australe quadrangle is also referred to as MC-30 (Mars Chart-30). [1] The quadrangle covers all the area of Mars south of 65°, including the South polar ice cap, and its ...
The Mare Acidalium quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The quadrangle is located in the northeastern portion of Mars' western hemisphere and covers 300° to 360° east longitude (0° to 60° west longitude) and 30° to 65° north latitude.
In March 2015, a team of scientists published results showing that this region was highly enriched with deuterium, heavy hydrogen, by seven times as much as the Earth. This means that Mars has lost a volume of water 6.5 times what is stored in today's polar caps. The water for a time would have formed an ocean in the low-lying Mare Boreum.
A 1962 map of Mars published by the U.S. Aeronautical Chart and Information Center, showing canals snaking through the Martian landscape. At the time, the existence of canals was still highly controversial as no close-up pictures of Mars had been taken (until Mariner 4 's flyby in 1965).
Map showing estimated water depth in different parts of Eridania Sea This map is about 530 miles across. Features around Eridania Sea labeled Research with CRISM found thick deposits, greater than 400 meters thick, that contained the minerals saponite , talc-saponite, Fe-rich mica (for example, glauconite - nontronite ), Fe- and Mg-serpentine ...
Montes Caucasus and closer structures with mineral postprocessing Detail map of Mare Imbrium's features. Montes Caucasus is marked "O". Montes Caucasus is a rugged range of mountains in the northeastern part of the Moon. [2]
Mare Fecunditatis / f ɪ ˌ k ʌ n d ɪ ˈ t eɪ t ɪ s / (Latin fēcunditātis, the "Sea of Fecundity" or "Sea of Fertility") is a lunar mare in the eastern half of the visible Moon. The mare has a maximum diameter of 840 km. [ 1 ]
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