Search results
Results From The WOW.Com Content Network
A STL 3D model of Mars with 20× elevation exaggeration using data from the Mars Global Surveyor Mars Orbiter Laser Altimeter. Mars, 2001, with the southern polar ice cap visible on the bottom. North Polar region with icecap. Across a whole planet, generalisation is not possible, and the geography of Mars varies considerably.
Listed are the elevations of the peaks (the vertical position relative to the areoid, which is the Martian vertical datum — the surface defined as zero elevation by average martian atmospheric pressure and planet radius), which is not the height above the surrounding terrain (topographic prominence). Listed mons elevation is the highest point ...
The northern part is an enormous topographic depression. About one-third of the surface (mostly in the northern hemisphere) lies 3–6 km lower in elevation than the southern two-thirds. This is a first-order relief feature on par with the elevation difference between Earth's continents and ocean basins. [12]
MOLA elevation map from the Mars Global Surveyor Mars orbiter Orcus Patera is a region on the surface of the planet Mars first photographed by Mariner 4 . Of unknown formation, whether by volcanic, tectonic, or cratering causes, the region includes a depression about 380 kilometres (240 miles) long, 140 kilometres (87 miles) wide, surrounded by ...
Ore resources on Mars – Ore deposits on Mars that may be useful to future colonists; Outflow channels – Long, wide swathes of scoured ground on Mars; Valley network (Mars) – Branching networks of valleys on Mars; Vallis – Valley landform on other planets; Water on Mars – Study of past and present water on Mars
The most conspicuous feature of Mars is a sharp contrast, known as the Martian dichotomy, between the Southern and the Northern hemispheres.The two hemispheres' geography differ in elevation by 1 to 3 km.
Elysium Mons / ɪ ˈ l ɪ z i ə m ˈ m ɒ n z / is a volcano on Mars located in the volcanic province Elysium, at , in the Martian eastern hemisphereIt stands about 12.6 km (41,000 ft) above its base, [2] and about 14.1 km (46,000 ft) above the Martian datum, [2] making it the third tallest Martian mountain in terms of relief and the fourth highest in elevation.
Mars is the fourth planet from the Sun.The surface of Mars is orange-red because it is covered in iron(III) oxide dust, giving it the nickname "the Red Planet". [22] [23] Mars is among the brightest objects in Earth's sky, and its high-contrast albedo features have made it a common subject for telescope viewing.