قائمة أطول الجبال في المجموعة الشمسية
القائمة

مذكور المرتفعات من «القاعدة إلى الذروة»، لأنه لا يوجد مكافئ للارتفاع فوق مستوى سطح البحر في عوالم أخرى.
| العالم | أعلى قمة (قمم) | ارتفاع "القاعدة إلى الذروة" | % نسبة الارتفاع إلى نصف القطر | سبب تكونه | ملاحظات |
| --- | --- | --- | --- | --- | --- |
| 01 !عطارد | Caloris Montes | 030 !≤ 3 كـم (1.9 ميل) | 0123 !0.12 | impact  | Formed by the Caloris impact |
| 02 !الزهرة | Skadi Mons (Maxwell Montes massif) | 064 !6.4 كـم (4.0 ميل) (11 km above mean) | 0106 !0.11 | tectonic | Has radar-bright slopes due to metallic Venus snow, possibly lead sulfide |
| 02 !الزهرة | Maat Mons | 049 !4.9 كـم (3.0 ميل) (approx.) | 0081 !0.081 | volcanic | Highest volcano on Venus |
|  الأرض | Mauna Kea and Mauna Loa | 102 !10.2 كـم (6.3 ميل) | 0160 !0.16 | volcanic | Just 4.2 كيلومتر (2.6 ميل) of this is above sea level |
|  الأرض | Haleakala | 091 !9.1 كـم (5.7 ميل) | 0142 !0.14 | volcanic | Rises 3.1 km above sea level |
|  الأرض | Pico del Teide | 075 !7.5 كـم (4.7 ميل) | 0118 !0.12 | volcanic | Rises 3.7 km above sea level |
|  الأرض | Denali | 056 !5.3 إلى 5.9 كـم (3.3 إلى 3.7 ميل) | 0093 !0.093 | tectonic | Tallest mountain base-to-peak on land |
|  الأرض | Mount Everest | 041 !3.6 إلى 4.6 كـم (2.2 إلى 2.9 ميل) | 0072 !0.072 | tectonic | 4.6 km on north face, 3.6 km on south face; highest elevation (8.8 km) above sea level (but not among the tallest from base to peak) |
| 04 !Moon | Mons Huygens | 055 !5.5 كـم (3.4 ميل) | 0317 !0.32 | impact | Formed by the Imbrium impact |
| 04 !Moon | Mons Hadley | 045 !4.5 كـم (2.8 ميل) | 0259 !0.26 | impact | Formed by the Imbrium impact |
| 04 !Moon | Mons Rümker | 011 !1.1 كـم (0.68 ميل) | 0063 !0.063 | volcanic | Largest volcanic construct on the Moon |
| 05 !Mars | Olympus Mons | 219 !21.9 كـم (14 ميل) | 0646 !0.65 | 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. |
| 05 !Mars | Ascraeus Mons | 149 !14.9 كـم (9.3 ميل) | 0440 !0.44 | volcanic | Tallest of the three Tharsis Montes |
| 05 !Mars | Elysium Mons | 126 !12.6 كـم (7.8 ميل) | 0372 !0.37 | volcanic | Highest volcano in Elysium |
| 05 !Mars | Arsia Mons | 117 !11.7 كـم (7.3 ميل) | 0345 !0.35 | volcanic | Summit caldera is 108 إلى 138 كيلومتر (67 إلى 86 ميل) across |
| 05 !Mars | Pavonis Mons | 084 !8.4 كـم (5.2 ميل) | 0248 !0.25 | volcanic | Summit caldera is 4.8 كيلومتر (3.0 ميل) deep |
| 05 !Mars | Anseris Mons | 062 !6.2 كـم (3.9 ميل) | 0183 !0.18 | impact | Among the highest nonvolcanic peaks on Mars, formed by the Hellas impact |
| 05 !Mars | Aeolis Mons ("Mount Sharp") | 050 !4.5 إلى 5.5 كـم (2.8 إلى 3.4 ميل) | 0162 !0.16 | deposition and erosion | Formed from deposits in Gale crater؛ the MSL rover has been ascending it since November 2014. |
| 06 !4 فيستا | Rheasilvia central peak | 220 !22 كـم (14 ميل) | 8370 !8.4 | impact | Almost 200 كيلومتر (120 ميل) wide. See also: List of largest craters in the Solar System |
| 07 !سيريس | Ahuna Mons | 040 !4 كـم (2.5 ميل) | 0853 !0.85 | 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 |
| 08 !Io | Boösaule Montes "South" | 178 !17.5 إلى 18.2 كـم (10.9 إلى 11.3 ميل) | 0999 !1.0 | tectonic | Has a 15 كيلومتر (9 ميل) high scarp on its SE margin |
| 08 !Io | Ionian Mons east ridge | 127 !12.7 كـم (7.9 ميل) (approx.) | 0697 !0.70 | tectonic | Has the form of a curved double ridge |
| 08 !Io | Euboea Montes | 118 !10.3 إلى 13.4 كـم (6.4 إلى 8.3 ميل) | 0736 !0.74 | tectonic | A NW flank landslide left a 25,000 km3 debris apron |
| 08 !Io | unnamed (245° W, 30° S) | 025 !2.5 كـم (1.6 ميل) (approx.) | 0137 !0.14 | volcanic | One of the tallest of Io's many volcanoes, with an atypical conical form |
| 09 !ميماس | Herschel central peak | 070 !7 كـم (4 ميل) (approx.) | 3530 !3.5 | impact | See also: List of largest craters in the Solar System |
| 10 !ديون | Janiculum Dorsa | 015 !1.5 كـم (0.9 ميل) | 0267 !0.27 | tectonic | Surrounding crust depressed ca. 0.3 km. |
| 11 !تيتان | Mithrim Montes | 033 !≤ 3.3 كـم (2.1 ميل) | 0130 !0.13 | tectonic | May have formed due to global contraction |
| 11 !تيتان | Doom Mons | 014 !1.45 كـم (0.90 ميل) | 0056 !0.056 | cryovolcanic | Adjacent to Sotra Patera, a 1.7 كيلومتر (1.1 ميل) deep collapse feature |
| 12 !إيابيتوس | equatorial ridge | 200 !20 كـم (12 ميل) (approx.) | 2720 !2.7 | uncertain | Individual peaks have not been measured |
| 13 !أوبيرون | unnamed ("limb mountain") | 110 !11 كـم (7 ميل) (approx.) | 1440 !1.4 | impact (?) | A value of 6 km was given shortly after the Voyager 2 encounter |
| 14 !بلوتو | Tenzing Montes, peak "T2" | 062 !~6.2 كـم (3.9 ميل) | 0522 !0.52 | tectonic (?) | Composed of water ice; named after Tenzing Norgay |
| 14 !بلوتو | Piccard Mons | 055 !~5.5 كـم (3.4 ميل) | 0463 !0.46 | cryovolcanic (?) | ~220 km across; central depression is 11 km deep |
| 14 !بلوتو | Wright Mons | 047 !~4.7 كـم (2.9 ميل) | 0396 !0.40 | cryovolcanic (?) | ~160 km across; summit depression ~56 km across and 4.5 km deep |
| 15 !شارون | Butler Mons | 045 !≥ 4.5 كـم (2.8 ميل) | 0743 !0.74 | tectonic (?) | Vulcan Planitia, the southern plains, has several isolated peaks, possibly tilted crustal blocks |
| 15 !شارون | Dorothy central peak | 040 !~4.0 كـم (2.5 ميل) | 0660 !0.66 | impact | North polar impact basin Dorothy, Charon's largest, is ∼240 km across and 6 km deep |