enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. List of montes on Venus - Wikipedia

    en.wikipedia.org/wiki/List_of_montes_on_Venus

    The four main mountain ranges of Venus are named Akna Montes, Danu Montes, Freyja Montes, and Maxwell Montes. These are found on Ishtar Terra. Mountain ranges are formed by the folding and buckling of a planet's crust. The mountain ranges of Venus, like those of the Earth, are characterized by many parallel folds and faults.

  3. Maxwell Montes - Wikipedia

    en.wikipedia.org/wiki/Maxwell_Montes

    The origin of the Lakshmi Planum and the mountain belts such as Maxwell Montes is controversial. One theory suggests they formed over a hot plume of material rising from Venus's interior, while another says the region is being compressed (pushed together) from all sides, resulting in material descending into the planet's interior. [5]

  4. Mons (planetary nomenclature) - Wikipedia

    en.wikipedia.org/wiki/Mons_(planetary_nomenclature)

    As of May 2015, 262 extraterrestrial mountains and mountain systems have official names: 117 on Venus, 50 on Mars, 48 on the Moon, 23 on Io, 13 on Titan, 9 on Iapetus, 1 on Mercury and 1 on Tethys. [3] They are named differently on different celestial bodies: [3] [13]

  5. List of tallest mountains in the Solar System - Wikipedia

    en.wikipedia.org/wiki/List_of_tallest_mountains...

    Olympus Mons, the tallest planetary mountain in the Solar System, compared to Mount Everest and Mauna Kea on Earth (heights shown are above datum or sea level, which differ from the base-to-peak heights given in the list). This is a list of the tallest mountains in the Solar System.

  6. Equatorial ridge on Iapetus - Wikipedia

    en.wikipedia.org/wiki/Equatorial_ridge_on_Iapetus

    The equatorial ridge is the tallest mountain feature on Saturn's moon Iapetus. It is 20 km (12 mi) high, and is the third tallest mountain structure in the Solar System. It runs along most of Iapetus' equator. It was discovered by the Cassini probe in 2004. The ridge's origin is unknown.

  7. Geology of Venus - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Venus

    The surface of Venus is comparatively flat. When 93% of the topography was mapped by Pioneer Venus Orbiter, scientists found that the total distance from the lowest point to the highest point on the entire surface was about 13 kilometres (8.1 mi), about the same as the vertical distance between the Earth's ocean floor and the higher summits of the Himalayas.

  8. Ishtar Terra - Wikipedia

    en.wikipedia.org/wiki/Ishtar_Terra

    Topographic radar image view of Venus, with Ishtar Terra near center. Ishtar Terra / ˈ ɪ ʃ t ɑːr ˈ t ɛr ə / [1] is the second largest of the three continental terrae regions on the planet Venus, the others being Aphrodite Terra and Lada Terra. It is a highland region named after the Akkadian goddess Ishtar, [2] and is found in the north ...

  9. Equatorial ridge - Wikipedia

    en.wikipedia.org/wiki/Equatorial_ridge

    Equatorial ridges are a feature of at least three of Saturn's moons: the large moon Iapetus and the tiny moons Atlas and Pan. They are ridges that closely follow the moons' equators. They appear to be unique to the Saturnian system, but it is uncertain whether the occurrences are related or a coincidence.