enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Olympus Mons - Wikipedia

    en.wikipedia.org/wiki/Olympus_Mons

    The Tharsis Montes are slightly smaller than Olympus Mons. A wide, annular depression or moat about 2 km (1.2 mi) deep surrounds the base of Olympus Mons and is thought to be due to the volcano's immense weight pressing down on the Martian crust. The depth of this depression is greater on the northwest side of the mountain than on the southeast ...

  3. Volcanism on Mars - Wikipedia

    en.wikipedia.org/wiki/Volcanism_on_Mars

    However, the largest volcano on the planet, Olympus Mons, is thought to have formed when the plates were not moving. Olympus Mons may have formed just after the plate motion stopped. The mare-like plains on Mars are roughly 3 to 3.5 billion years old. [72] The giant shield volcanoes are younger, formed between 1 and 2 billion years ago.

  4. Tharsis - Wikipedia

    en.wikipedia.org/wiki/Tharsis

    Tharsis (/ ˈ θ ɑːr s ɪ s /) is a vast volcanic plateau centered near the equator in the western hemisphere of Mars. [note 1] The region is home to the largest volcanoes in the Solar System, including the three enormous shield volcanoes Arsia Mons, Pavonis Mons, and Ascraeus Mons, which are collectively known as the Tharsis Montes.

  5. List of mountains on Mars - Wikipedia

    en.wikipedia.org/wiki/List_of_mountains_on_Mars

    Mons — large, isolated, mountain; may or may not be of volcanic origin. plural montes — mountain range. Tholus — small dome-shaped mountain or hill. plural tholi — group of (usually not contiguous) small mountains. Dorsum — long low range. Name type not present on Mars. plural dorsa

  6. Tharsis Montes - Wikipedia

    en.wikipedia.org/wiki/Tharsis_Montes

    Mons (plural montes) is the Latin word for mountain; it is a descriptor term used in astrogeology for mountainous features in the Solar System. The three Tharsis Montes volcanoes are enormous by terrestrial standards, ranging in diameter from 375 km (233 mi) (Pavonis Mons) to 475 km (295 mi) (Arsia Mons). [1]

  7. Evidence of water on Mars found by Mars Reconnaissance ...

    en.wikipedia.org/wiki/Evidence_of_water_on_Mars...

    The layering is believed to have come from the global warming and cooling cycle on Mars; during cooling periods, water migrated to the poles and formed the ice-water layers, while on subsequent warming, the unthawed ice water was covered by layers of dust and dirt from windstorms on the surface, helping to preserve the ice water. [44] [45]

  8. Amazonis quadrangle - Wikipedia

    en.wikipedia.org/wiki/Amazonis_quadrangle

    The central part contains Amazonis Planitia and the eastern part includes the western flank of the largest known volcano in the Solar System, Olympus Mons. The Amazonis quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program .

  9. Noctis Labyrinthus - Wikipedia

    en.wikipedia.org/wiki/Noctis_Labyrinthus

    Noctis Labyrinthus is located in the heart of Tharsis at the western end of the Valles Marineris, manifesting as a network of graben that extends in a spider-like network before coalescing into a coherent, relatively shallow graben swarm that curves in a semicircular fashion towards the south into the Claritas Rise.

  1. Related searches is olympus mons explosive or non polar water cooler not cooling better than normal

    olympus mons viewolympus mons elevation
    olympus mons wikipediawhere is olympus mons
    map of olympus monsflanks of olympus mons
    depth of olympus mons