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Tallest mountain base-to-peak on land [15] [n 3] Mount Everest: 3.6 to 4.6 km (2.2 to 2.9 mi) [16] 0.072: tectonic: 4.6 km on north face, 3.6 km on south face; [n 4] highest elevation (8.8 km) above sea level, as well as by wet and dry prominence (but not among the tallest from base to peak, and in distance to Earth's center Mt Chimborazo rises ...
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.
In 1978, the space probe Pioneer Venus 1 went into orbit around Venus for the purpose of making radar observations of the Venusian surface. These observations made possible the creation of the first topographic map of the surface of Venus, and confirmed that a point within Maxwell Montes is the highest point above the average level of the ...
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.
This is a list of montes (mountains, singular mons) on the planet Venus. Venusian mountains are all named after goddesses in the mythologies of various cultures, except for the Maxwell Montes. The four main mountain ranges of Venus are named Akna Montes, Danu Montes, Freyja Montes, and Maxwell Montes. These are found on Ishtar Terra.
An area of tile-like, polygonal terrain. This term is used only on Venus. TE Tholus, tholi / ˈ θ oʊ l ə s /, / ˈ θ oʊ l aɪ / Small domical mountain or hill e.g. Hecates Tholus. TH Undae, undae / ˈ ʌ n d iː / A field of dunes. Used on Venus, Mars and Titan. UN Vallis, valles / ˈ v æ l ɪ s /, / ˈ v æ l iː z / A valley e.g. Valles ...
Once Venus enters your sign on Feb. 4, your charm and magnetism get a significant boost, making you feel like the center of attention. This is your time to shine, especially with matters of the ...
The Galilean satellites show a similar trend going outwards from Jupiter; however, no such trend is observable for the icy satellites of Saturn or Uranus. [12] The icy worlds typically have densities less than 2 g·cm −3. Eris is significantly denser (2.43 ± 0.05 g·cm −3), and may be mostly rocky with some surface ice, like Europa. [2]