List of tallest mountains in the Solar System
This is a list of the tallest mountains in the Solar System. The tallest peak or peaks on worlds where significant mountains have been measured are given. For some worlds, the tallest peaks of different classes are also listed. At 21.9 km, the enormous shield volcano Olympus Mons on Mars is the tallest mountain on any planet in the Solar System. For 40 years, following its discovery in 1971, it was the tallest mountain known in the Solar System. However, in 2011, the central peak of the crater Rheasilvia on the asteroid and protoplanet Vesta was found to be of comparable height. Due to limitations in the data and the definition problem described below, it is difficult to determine which of the two is taller.
List
Heights are given from base to peak. Peak elevations above sea level are only available on Earth, and possibly Titan. On other worlds, peak elevations above an equipotential surface or a reference ellipsoid could be used if enough data is available for the calculation, but this is often not the case.World | Tallest peak | Base-to-peak height | % of radius | Origin | Notes |
Caloris Montes | impact | Formed by the Caloris impact | |||
Skadi Mons | tectonic | Has radar-bright slopes due to metallic Venus snow, possibly lead sulfide | |||
Maat Mons | volcanic | Highest volcano on Venus | |||
Earth | Mauna Kea and Mauna Loa | volcanic | Just of this is above sea level | ||
Earth | Haleakala | volcanic | Rises 3.1 km above sea level | ||
Earth | Pico del Teide | volcanic | Rises 3.7 km above sea level | ||
Earth | Denali | tectonic | Tallest mountain base-to-peak on land | ||
Earth | Mount Everest | tectonic | 4.6 km on north face, 3.6 km on south face; highest elevation above sea level | ||
Mons Huygens | impact | Formed by the Imbrium impact | |||
Mons Hadley | impact | Formed by the Imbrium impact | |||
Mons Rümker | volcanic | Largest volcanic construct on the Moon | |||
Olympus Mons | volcanic | Rises 26 km above northern plains, 1000 km away. Summit calderas are 60 x 80 km wide, up to 3.2 km deep; scarp around margin is up to 8 km high. A shield volcano, the mean flank slope is a modest 5.2 degrees. | |||
Ascraeus Mons | volcanic | Tallest of the three Tharsis Montes | |||
Elysium Mons | volcanic | Highest volcano in Elysium | |||
Arsia Mons | volcanic | Summit caldera is across | |||
Pavonis Mons | volcanic | Summit caldera is deep | |||
Anseris Mons | impact | Among the highest nonvolcanic peaks on Mars, formed by the Hellas impact | |||
Aeolis Mons | deposition and erosion | Formed from deposits in Gale crater; the MSL rover has been ascending it since November 2014. | |||
Rheasilvia central peak | impact | Almost wide. See also: List of largest craters in the Solar System | |||
Ahuna Mons | cryovolcanic | Isolated steep-sided dome in relatively smooth area; max. height of ~ 5 km on steepest side; roughly antipodal to largest impact basin on Ceres | |||
Boösaule Montes "South" | tectonic | Has a high scarp on its SE margin | |||
Ionian Mons east ridge | tectonic | Has the form of a curved double ridge | |||
Euboea Montes | tectonic | A NW flank landslide left a 25,000 km3 debris apron | |||
unnamed | volcanic | One of the tallest of Io's many volcanoes, with an atypical conical form | |||
Herschel central peak | impact | See also: List of largest craters in the Solar System | |||
Janiculum Dorsa | tectonic | Surrounding crust depressed ca. 0.3 km. | |||
Mithrim Montes | tectonic | May have formed due to global contraction | |||
Doom Mons | cryovolcanic | Adjacent to Sotra Patera, a deep collapse feature | |||
equatorial ridge | uncertain | Individual peaks have not been measured | |||
unnamed | impact | A value of 6 km was given shortly after the Voyager 2 encounter | |||
Tenzing Montes, peak "T2" | tectonic | Composed of water ice; named after Tenzing Norgay | |||
Piccard Mons | cryovolcanic | ~220 km across; central depression is 11 km deep | |||
Wright Mons | cryovolcanic | ~160 km across; summit depression ~56 km across and 4.5 km deep | |||
Butler Mons | tectonic | Vulcan Planitia, the southern plains, has several isolated peaks, possibly tilted crustal blocks | |||
Dorothy central peak | impact | North polar impact basin Dorothy, Charon's largest, is ∼240 km across and 6 km deep |