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| [[Tập tin:Iapetus equatorial ridge.jpg|40px]]
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{| class="wikitable sortable"
|-
! width="30" |Hành tinh <br />hoặc vệ tinh
! class=unsortable|Mỏm cao <br />nhất
! width="189" |Chiều cao
! width="20" |% of radius{{refn |100 x ratio of peak height to '''radius of the parent world'''| group = n }}
! width="84" |Origin
! Hình ảnh
!class=unsortable|Notes
|-
| {{hs|01}} [[Mercury (planet)|Mercury]] || [[Caloris Montes]] || {{hs|030}}≤ {{convert|abbr=on|3|km|mi|1}}<ref>{{cite web
| title = Surface
| work = MESSENGER web site
| publisher = [[Johns Hopkins University]]/[[Applied Physics Lab]]
| url = http://messenger-education.org/elusive_planet/surface.htm
| accessdate = 4 April 2012}}</ref><ref name="OberstPreusker2010">{{cite journal|last1=Oberst|first1=J.|last2=Preusker|first2=F.|last3=Phillips|first3=R. J.|last4=Watters|first4=T. R.|last5=Head|first5=J. W.|last6=Zuber|first6=M. T.|last7=Solomon|first7=S. C.|title=The morphology of Mercury’s Caloris basin as seen in MESSENGER stereo topographic models|journal=Icarus |volume=209|issue=1 |date=2010|pages=230–238 |issn=0019-1035|doi=10.1016/j.icarus.2010.03.009|bibcode = 2010Icar..209..230O }}</ref>
| {{hs|0123}} 0.12
| [[Impact crater|impact]]<ref name="FassettHead2009">{{cite journal|last1=Fassett|first1=C. I.|last2=Head|first2=J. W.|last3=Blewett|first3=D. T.|last4=Chapman|first4=C. R.|last5=Dickson|first5=J. L.|last6=Murchie|first6=S. L.|last7=Solomon|first7=S. C.|last8=Watters|first8=T. R.|title=Caloris impact basin: Exterior geomorphology, stratigraphy, morphometry, radial sculpture, and smooth plains deposits|journal=Earth and Planetary Science Letters|volume=285 |issue=3-4|date=2009 |pages=297–308|issn=0012-821X |doi=10.1016/j.epsl.2009.05.022|bibcode = 2009E&PSL.285..297F }}</ref>
| Formed by the [[Caloris Basin|Caloris impact]]
|-
| rowspan="2" | {{hs|02}} [[List of montes on Venus|Venus]]
| [[Skadi Mons]]
| {{hs|064}}{{convert|abbr=on|6.4|km|mi|1}} (approx.)<ref name = "planetology">{{cite book| title = Planetology : Unlocking the secrets of the solar system|author1=Jones, Tom |author2=Stofan, Ellen | date = 2008| publisher = National Geographic Society| location = Washington, D.C.| page = 74| isbn = 978-1-4262-0121-9| url = https://books.google.com/books?id=SL-BszT15s0C&pg=PA74}}</ref>
| {{hs|0106}} 0.11
| [[Orogeny|tectonic]]<ref name="KeepHansen1994">{{cite journal|last1=Keep|first1=M.| last2=Hansen|first2=V. L.|title=Structural history of Maxwell Montes, Venus: Implications for Venusian mountain belt formation|journal=Journal of Geophysical Research| volume=99|issue=E12| date=1994|pages=26015| issn=0148-0227| doi=10.1029/94JE02636|bibcode = 1994JGR....9926015K }}</ref>
| Has radar-bright slopes due to metallic [[Venus snow]], possibly [[Galena|lead sulfide]]<ref name="wustl-lead-sulfide">{{cite news
|title= 'Heavy metal' snow on Venus is lead sulfide
|last= Otten |first= Carolyn Jones
|url= http://news.wustl.edu/news/Pages/633.aspx
|publisher= [[Washington University in Saint Louis]]
|newspaper= Newsroom
|date= 10 February 2004 |accessdate= 10 December 2012
}}</ref>
|-
| [[Maat Mons]]
| {{hs|049}}{{convert|abbr=on|4.9|km|mi|1}} (approx.)<ref name = "Maat">{{cite web
| title = PIA00106: Venus - 3D Perspective View of Maat Mons
| work = Planetary Photojournal
| publisher = [[Jet Propulsion Lab]]
| date = 1996-08-01
| url = http://photojournal.jpl.nasa.gov/catalog/PIA00106
| accessdate = 30 June 2012}}</ref>
| {{hs|0081}} 0.081
| [[Volcano|volcanic]]<ref name = "">{{cite journal |last=Robinson |first=C. A. |author2=Thornhill, G. D. |author3=Parfitt, E. A. |date=January 1995 |title=Large-scale volcanic activity at Maat Mons: Can this explain fluctuations in atmospheric chemistry observed by Pioneer Venus? |journal=Journal of Geophysical Research |volume=100 |issue = E6 |pages=11755–11764 |url=http://www.agu.org/pubs/crossref/1995/95JE00147.shtml |accessdate= 11 February 2013 |doi=10.1029/95JE00147 |bibcode=1995JGR...10011755R}}</ref>
| Highest volcano on Venus
|-
| rowspan="5" | {{hs|03}} [[List of highest mountains|Earth]]
| [[Mauna Kea]] and [[Mauna Loa]]<!--they are effectively the same height at this scale-->
| {{hs|102}}{{convert|abbr=on|10.2|km|mi|1}}<ref name = "Highest_Points">{{cite web |url=http://science.nationalgeographic.com/science/earth/surface-of-the-earth/mountains-article/ |title=Mountains: Highest Points on Earth |publisher=National Geographic Society |accessdate=19 September 2010}}</ref>
| {{hs|0160}} 0.16
| [[Volcano|volcanic]]
| Just {{convert|abbr=on|4.2|km|mi|1}} of this is above sea level
|-
| [[Haleakala]]
| {{hs|091}}{{convert|abbr=on|9.1|km|mi|1}}<ref name = "NPS">{{cite web
| title = Haleakala National Park Geology Fieldnotes| last = | first =
| publisher = U.S. National Park Service | url = https://www.nature.nps.gov/geology/parks/hale/index.cfm
| accessdate = 31 January 2017}}</ref>
| {{hs|0142}} 0.14
| [[Volcano|volcanic]]
| Rises 3.1&nbsp;km above sea level<ref name = "NPS" />
|-
| [[Teide|Pico del Teide]]
| {{hs|075}}{{convert|abbr=on|7.5|km|mi|1}}<ref name = "UNESCO">{{cite web
| title = Teide National Park | work = UNESCO World Heritage Site list
| publisher = [[UNESCO]] | url = http://whc.unesco.org/en/list/1258
| accessdate = 2 June 2013}}</ref>
| {{hs|0118}} 0.12
| [[Volcano|volcanic]]
| Rises 3.7&nbsp;km above sea level<ref name = "UNESCO"/>
|-
| [[Denali]]
| {{hs|056}}{{convert|abbr=on|5.3|to|5.9|km|mi|1}}<ref>{{cite web|url=https://www.pbs.org/wgbh/nova/denali/expedition/mission.html|title=NOVA Online: Surviving Denali, The Mission|publisher=Public Broadcasting Corporation|work=NOVA web site|date=2000|accessdate=7 June 2007}}</ref>
| {{hs|0093}} 0.093
| [[Orogeny|tectonic]]
| Tallest mountain base-to-peak on land<ref name="Helman2005">{{cite book|author=Adam Helman|title=The Finest Peaks: Prominence and Other Mountain Measures|url=https://books.google.com/books?id=kr8AM-w8IFQC&printsec=frontcover |accessdate=9 December 2012|date=2005|publisher=Trafford Publishing|isbn=978-1-4120-5995-4}}</ref>{{refn |On p. 20 of Helman (2005): "the base to peak rise of Mount McKinley is the largest of any mountain that lies entirely above sea level, some {{convert|18000|feet|meter|abbr=on}}"| group = n }}
|-
| [[Mount Everest]]
| {{hs|041}}{{convert|abbr=on|3.6|to|4.6|km|mi|1}}<ref name="washburn_map">''Mount Everest'' (1:50,000 scale map), prepared under the direction of [[Bradford Washburn]] for the Boston Museum of Science, the Swiss Foundation for Alpine Research, and the [[National Geographic Society]], 1991, {{ISBN|3-85515-105-9}}</ref>
| {{hs|0072}} 0.072
| [[Orogeny|tectonic]]
| 4.6&nbsp;km on north face, 3.6&nbsp;km on south face;{{refn |Peak is {{convert|abbr=on|8.8|km|mi|1}} above sea level, and over {{convert|abbr=on|13|km|mi|1}} above the oceanic [[abyssal plain]].| group = n }} listed only because it has the highest elevation (8.8 km) above sea level
<!-- K2 is probably not #4 |-
| [[K2]]
| {{hs|028}}{{convert|abbr=on|2.8|to|3.2|km|mi|1}} -->
|-
| rowspan="3" | {{hs|04}} [[Mặt Trăng]]
| [[Mons Huygens]]
| {{hs|055}}{{convert|abbr=on|5.5|km|mi|1}}<ref name="price"/><ref name="moore"/>
| {{hs|0317}} 0.32
| [[Impact crater|impact]]
| [[Tập tin:Apennines.jpg|40px]]
| Formed by the [[Mare Imbrium|Imbrium impact]]
|-
| [[Mons Hadley]]
| {{hs|045}}{{convert|abbr=on|4.5|km|mi|1}}<ref name="price">{{cite book | author=Fred W. Price | title=The Moon observer's handbook | publisher=Cambridge University Press | location=London | date=1988 | isbn= 0-521-33500-0}}</ref><ref name="moore">{{cite book | last=Moore | first=Patrick | authorlink = Patrick Moore | title=On the Moon | publisher=Cassell & Co | location=London | date=2001 }}</ref>
| {{hs|0259}} 0.26
| [[Impact crater|impact]]
| Formed by the [[Mare Imbrium|Imbrium impact]]
|-
| [[Mons Rümker]]
| {{hs|011}}{{convert|abbr=on|1.1|km|mi|2}}<ref name="laps07">{{Citation
|author1=Wöhler, C. |author2=Lena, R. |author3=Pau, K. C. | title=The Lunar Dome Complex Mons Rümker: Morphometry, Rheology, and Mode of Emplacement
| booktitle=Proceedings Lunar and Planetary Science XXXVIII
| publisher=Dordrecht, D. Reidel Publishing Co
| date=16 March 2007 | location=League City, Texas
| url=http://labs.adsabs.harvard.edu/ui/abs/2007LPI....38.1091W?
| accessdate = 28 August 2007 }}</ref>
| {{hs|0063}} 0.063
| [[Volcano|volcanic]]
| Largest volcanic construct on the Moon<ref name="laps07"/>
|-
| rowspan=7|{{hs|05}} [[List of mountains on Mars by height|Mars]]
| [[Olympus Mons]]
| {{hs|219}} {{convert|abbr=on|21.9|km|mi|0}}<ref name="Plescia2004">{{cite journal|last1=Plescia|first1=J. B.|title=Morphometric properties of Martian volcanoes|journal=Journal of Geophysical Research|volume=109|issue=E3|date=2004|issn=0148-0227|doi=10.1029/2002JE002031|bibcode = 2004JGRE..109.3003P }}</ref><ref name="Carr2007" />
| {{hs|0646}} 0.65
| [[Volcano|volcanic]]
| Rises 26&nbsp;km above northern plains,<ref name="Comins2012">{{cite book|last=Comins|first=Neil F.| title=Discovering the Essential Universe|url=https://books.google.com/books?id=qK_4mNve1DYC&pg=PA148&dq=mons+olympus+height&hl=en&sa=X&ei=YzCQT-GpIcH22AXz852ABQ&ved=0CDoQ6AEwAQ#v=onepage&q=mons%20olympus%20height&f=false|accessdate=23 December 2012|date=4 January 2012|publisher=Macmillan|isbn=978-1-4292-5519-6}}</ref> 1000&nbsp;km away. Summit calderas are 60 x 80 km wide, up to 3.2 km deep;<ref name="Carr2007">{{cite book|author=Carr, Michael H.|title=The Surface of Mars|url=https://books.google.com/books?id=uLHlJ6sjohwC|date=11 January 2007|publisher=Cambridge University Press|isbn=978-1-139-46124-5|page=51}}</ref> scarp around margin is up to 8 km high.<ref name="Lopes1982">{{cite journal|last1=Lopes|first1=R.|last2=Guest|first2=J. E.|last3=Hiller|first3=K.|last4= Neukum|first4= G.|title=Further evidence for a mass movement origin of the Olympus Mons aureole|journal=Journal of Geophysical Research|volume=87|issue= B12|date=January 1982|pages= 9917–9928|doi= 10.1029/JB087iB12p09917|bibcode=1982JGR....87.9917L}}</ref>
|-
| [[Ascraeus Mons]]
| {{hs|149}}{{convert|abbr=on|14.9|km|mi|1}}<ref name="Plescia2004"/>
| {{hs|0440}} 0.44
| [[Volcano|volcanic]]
| Tallest of the three [[Tharsis Montes]]
|-
| [[Elysium Mons]]
| {{hs|126}}{{convert|abbr=on|12.6|km|mi|1}}<ref name="Plescia2004"/>
| {{hs|0372}} 0.37
| [[Volcano|volcanic]]
| Highest volcano in [[Elysium (volcanic province)|Elysium]]
|-
| [[Arsia Mons]]
| {{hs|117}} {{convert|abbr=on|11.7|km|mi|1}}<ref name="Plescia2004"/>
| {{hs|0345}} 0.35
| [[Volcano|volcanic]]
| Summit [[caldera]] is {{convert|abbr=on|108|to|138|km|mi|0}} across<ref name="Plescia2004"/>
|-
| [[Pavonis Mons]]
| {{hs|084}} {{convert|abbr=on|8.4|km|mi|1}}<ref name="Plescia2004"/>
| {{hs|0248}} 0.25
| [[Volcano|volcanic]]
| Summit caldera is {{convert|abbr=on|4.8|km|mi|1}} deep<ref name="Plescia2004"/>
|-
| [[Anseris Mons]]
| {{hs|062}} {{convert|abbr=on|6.2|km|mi|1}}<ref name = "MOLA">JMARS MOLA elevation dataset. Christensen, P.; Gorelick, N.; Anwar, S.; Dickenshied, S.; Edwards, C.; Engle, E. (2007) "[http://adsabs.harvard.edu/abs/2007AGUFM.P11E..01C New Insights About Mars From the Creation and Analysis of Mars Global Datasets];" American Geophysical Union, Fall Meeting, abstract #P11E-01.</ref>
| {{hs|0183}} 0.18
| [[Impact crater|impact]]
| Among the highest nonvolcanic peaks on Mars, formed by the [[Hellas Planitia|Hellas impact]]
|-
| [[Aeolis Mons]] ("Mount Sharp")
| {{hs|050}} {{convert|abbr=on|4.5|to|5.5|km|mi|1}}<ref name="themis">{{cite web
| url = http://themis.asu.edu/features/galecrater
| title = Gale Crater's History Book
| work = Mars Odyssey THEMIS web site
| publisher=[[Arizona State University]]
| accessdate = 7 December 2012}}</ref>{{refn |About {{convert|5.25|km|mi|abbr=on}} high from the perspective of the landing site of ''Curiosity''.<ref name="Anderson2010">{{cite journal
|last=Anderson |first=R. B. |last2=Bell III |first2=J. F. |date=2010
|title=Geologic mapping and characterization of Gale Crater and implications for its potential as a Mars Science Laboratory landing site
|url=http://www.marsjournal.org/contents/2010/0004/
|journal=International Journal of Mars Science and Exploration
|volume=5 |issue= |pages=76–128 |bibcode=2010IJMSE...5...76A
|doi=10.1555/mars.2010.0004}}</ref> | group = n }}
| {{hs|0162}} 0.16
| [[Deposition (geology)|deposition]] and [[erosion]]{{refn|A crater central peak may sit below the mound of sediment. If that sediment was deposited while the crater was flooded, the crater may have once been entirely filled before [[erosion]]al processes gained the upper hand.<ref name="themis"/> However, if the deposition was due to [[katabatic wind]]s, as suggested by reported 3 degree radial slopes of the mound's layers, the role of erosion would have been to place an upper limit on the mound's growth.<ref name = "Wall_2013">{{cite web
| last = Wall | first = M.
| title = Bizarre Mars Mountain Possibly Built by Wind, Not Water
| publisher = [[Space.com]] | date = 6 May 2013
| url = http://www.space.com/20986-mars-mountain-water-formation.html
| accessdate = 13 May 2013}}</ref><ref name="KiteLewis2013">{{cite journal|last1=Kite|first1=E. S.|last2=Lewis|first2=K. W.|last3=Lamb|first3=M. P.|last4=Newman|first4=C. E.|last5=Richardson|first5=M. I.|title=Growth and form of the mound in Gale Crater, Mars: Slope wind enhanced erosion and transport|journal=Geology|volume= 41|issue=5|date= 2013|pages=543–546|issn= 0091-7613|doi= 10.1130/G33909.1|arxiv=1205.6840|bibcode=2013Geo....41..543K}}</ref>| group = n }}
| Formed from deposits in [[Gale (crater)|Gale crater]];<ref name="NASA-20120328">{{cite web |last=Agle |first=D. C. |title='Mount Sharp' On Mars Links Geology's Past and Future |url=http://www.nasa.gov/mission_pages/msl/news/msl20120328.html |date=28 March 2012 |publisher=[[NASA]] |accessdate=31 March 2012 }}</ref> the [[Curiosity (rover)|MSL rover]] has been ascending it since November 2014.<ref>{{cite news|last1=Webster|first1=Gay|last2=Brown|first2=Dwayne|title=Curiosity Arrives at Mount Sharp|url=http://mars.nasa.gov/msl/news/whatsnew/index.cfm?FuseAction=ShowNews&NewsID=1705|accessdate=16 October 2016|work=NASA Jet Propulsion Laboratory|date=9 November 2014}}</ref>
|-
| {{hs|06}} [[4 Vesta|Vesta]]
| [[Rheasilvia|Rheasilvia central peak]]
| {{hs|220}}{{convert|abbr=on|22|km|mi|0}}<ref name="Vega">{{cite web
|last=Vega
|first=P.
|title=New View of Vesta Mountain From NASA's Dawn Mission
|work=Jet Propulsion Lab's Dawn mission web site
|publisher=[[NASA]]
|date=11 October 2011
|url=http://dawn.jpl.nasa.gov/feature_stories/new_view_vesta_mountain.asp
|accessdate=29 March 2012
|deadurl=yes
|archiveurl=https://web.archive.org/web/20111022092700/http://dawn.jpl.nasa.gov/feature_stories/new_view_vesta_mountain.asp
|archivedate=22 October 2011
|df=
}}</ref><ref name = "Schenk_2012">{{Citation
| last1 = Schenk | first1 = P. | last2 = Marchi | first2 = S. | last3 = O'Brien | first3 = D. P. | last4 = Buczkowski | first4 = D. | last5 = Jaumann | first5 = R. | last6 = Yingst | first6 = A. | last7 = McCord | first7 = T. | last8 = Gaskell | first8 = R. | last9 = Roatsch | first9 = T. | last10 = Keller | first10 = H. E. | last11 = Raymond | first11 = C.A. | last12 = Russell | first12 = C. T.
| title = Mega-Impacts into Planetary Bodies: Global Effects of the Giant Rheasilvia Impact Basin on Vesta
| booktitle = 43rd Lunar and Planetary Science Conference
| id = contribution 1659, id.2757
| publisher = [[Lunar and Planetary Institute|LPI]]
| date = 1 March 2012
| location = The Woodlands, Texas
| url = http://adsabs.harvard.edu/abs/2012LPI....43.2757S
| accessdate = 6 September 2012}}</ref>
| {{hs|8370}} 8.4
| [[Impact crater|impact]]
| Almost {{convert|200|km|mi|abbr=on}} wide. See also: [[List of largest craters in the Solar System]]
|-
| {{hs|07}} [[Ceres (dwarf planet)|Ceres]]
| [[Ahuna Mons]]
| {{hs|040}}{{convert|abbr=on|4|km|mi|1}}<ref name = "Ceres">{{cite web
| title = Dawn's First Year at Ceres: A Mountain Emerges | website = JPL Dawn website
| publisher = [[Jet Propulsion Lab]] | date = 2016-03-07
| url = http://dawn.jpl.nasa.gov/news/news-detail.html?id=5745 | accessdate = 2016-03-08}}</ref>
| {{hs|0853}} 0.85
| [[cryovolcanic]]<ref name="Ruesch2016">{{cite journal|last1=Ruesch|first1= O.|last2=Platz|first2= T.|last3=Schenk|first3= P.|last4=McFadden|first4=L. A.|last5=Castillo-Rogez|first5=J. C.|last6=Quick|first6=L. C.|last7=Byrne|first7= S.|last8=Preusker|first8= F.|last9=OBrien|first9=D. P.|last10=Schmedemann|first10= N.|last11=Williams|first11=D. A.|last12=Li|first12=J.- Y.|last13=Bland|first13=M. T.|last14=Hiesinger|first14= H.|last15=Kneissl|first15=T.|last16=Neesemann|first16= A.|last17=Schaefer|first17= M.|last18=Pasckert|first18=J. H.|last19=Schmidt|first19=B. E.|last20=Buczkowski|first20=D. L.|last21=Sykes|first21=M. V.|last22=Nathues|first22= A.|last23=Roatsch|first23= T.|last24=Hoffmann|first24= M.|last25=Raymond|first25=C. A.|last26=Russell|first26=C. T.|title=Cryovolcanism on Ceres|journal= Science|volume= 353|issue= 6303|date= 2016-09-02|pages= aaf4286–aaf4286|doi= 10.1126/science.aaf4286|bibcode=2016Sci...353.4286R}}</ref>
| Isolated steep-sided dome in relatively smooth area; max. height of ~ 5 km on steepest side; roughly [[Antipodes|antipodal]] to [[Kerwan (crater)|largest impact basin on Ceres]]
|-
| rowspan="4" | {{hs|08}} [[List of mountains on Io|Io]]
| [[Boösaule Montes]] "South"<ref name = "Boösaule Montes">{{cite web
| last = Perry | first = Jason | title = Boösaule Montes
| work = Gish Bar Times blog
| publisher = | date = 27 January 2009
| url = http://www.gishbartimes.org/2009/01/boosaule-montes.html
| accessdate = 30 June 2012}}</ref>
| {{hs|178}}{{convert|abbr=on|17.5|to|18.2|km|mi|1}}<ref name = "Boösaule Montes2">{{cite web
| last = Schenk | first = P. | authorlink =
|author2=Hargitai, H.
| title = Boösaule Montes
| work = Io Mountain Database
| publisher = | url = http://planetologia.elte.hu/io/index.phtml?nev=271s10
| accessdate = 30 June 2012}}</ref>
| {{hs|0999}} 1.0
| [[Orogeny|tectonic]]
| Has a {{convert|abbr=on|15|km|mi|0}} high scarp on its SE margin<ref name="SchenkHargitai2001">{{cite journal|last1=Schenk|first1=P.|last2=Hargitai|first2=H.|last3=Wilson|first3=R.|last4=McEwen|first4=A.|last5=Thomas|first5=P.|title=The mountains of Io: Global and geological perspectives from Voyager and Galileo|journal= Journal of Geophysical Research|volume= 106|issue= E12|date= 2001|pages= 33201|issn=0148-0227|doi=10.1029/2000JE001408|bibcode = 2001JGR...10633201S }}</ref>
|-
| Ionian Mons east ridge
| {{hs|127}}{{convert|abbr=on|12.7|km|mi|1}} (approx.)<ref name="SchenkHargitai2001"/><ref name = "Ionian Mons">{{cite web
| last = Schenk | first = P. | authorlink =
|author2=Hargitai, H.
| title = Ionian Mons
| work = Io Mountain Database
| publisher = | url = http://planetologia.elte.hu/io/index.phtml?nev=236n08
| accessdate = 30 June 2012}}</ref>
| {{hs|0697}} 0.70
| [[Orogeny|tectonic]]
| Has the form of a curved double ridge
|-
| [[Euboea Montes]]
| {{hs|118}}{{convert|abbr=on|10.3|to|13.4|km|mi|1}}<ref name = "Euboea Montes">{{cite web
| last = Schenk | first = P. | authorlink =
|author2=Hargitai, H.
| title = Euboea Montes
| work = Io Mountain Database
| publisher = | url = http://planetologia.elte.hu/io/index.phtml?nev=335s47
| accessdate = 30 June 2012}}</ref>
| {{hs|0736}} 0.74
| [[Orogeny|tectonic]]
| A NW flank landslide left a 25,000&nbsp;km<sup>3</sup> debris apron<ref name = "Martel">{{cite web
| last = Martel | first = L. M. V. | title = Big Mountain, Big Landslide on Jupiter's Moon, Io
| work = NASA Solar System Exploration web site
| publisher =
| date = 16 February 2011
| url = http://solarsystem.nasa.gov/scitech/display.cfm?ST_ID=487
| accessdate = 30 June 2012}}</ref>{{refn |Among the Solar System's largest<ref name = "Martel"/>| group = n }}
|-
| unnamed (245° W, 30° S)
| {{hs|020}}{{convert|abbr=on|2.5|km|mi|1}} (approx.)<ref name="MooreMcEwen1986">{{cite journal|last1=Moore|first1=J. M.|last2=McEwen|first2=A. S.|last3=Albin|first3=E. F.|last4=Greeley|first4=R.|title=Topographic evidence for shield volcanism on Io|journal=Icarus |volume=67|issue=1 |date=1986|pages=181–183 |issn=0019-1035|doi=10.1016/0019-1035(86)90183-1|bibcode = 1986Icar...67..181M }}</ref><ref name = "unnamed_Io">{{cite web
| last = Schenk | first = P. | authorlink =
|author2=Hargitai, H.
| title = Unnamed volcanic mountain
| work = Io Mountain Database
| publisher = | url = http://planetologia.elte.hu/io/index.phtml?nev=245s29
| accessdate = 6 December 2012}}</ref>
| {{hs|013}} 0.14
| [[Volcano|volcanic]]
| One of the tallest of Io's many volcanoes, with an atypical conical form<ref name = "unnamed_Io"/>{{refn |Some of [[List of paterae on Io|Io's paterae]] are surrounded by radial patterns of lava flows, indicating they are on a topographic high point, making them shield volcanoes. Most of these volcanoes exhibit relief of less than 1 km. A few have more relief; [[Ruwa Patera]] rises 2.5 to 3 km over its 300 km width. However, its slopes are only on the order of a degree.<ref name="Schenk2004">{{cite journal | last=Schenk |first=P. M. |author2=Wilson, R. R. |author3=Davies, R. G. |title=Shield volcano topography and the rheology of lava flows on Io |journal=Icarus |volume=169 |issue= 1|pages=98–110 |date=2004 |url= |doi=10.1016/j.icarus.2004.01.015 |bibcode=2004Icar..169...98S}}</ref> A handful of Io's smaller shield volcanoes have steeper, conical profiles; the example listed is 60 km across and has slopes averaging 4° and reaching 6-7° approaching the small summit depression.<ref name="Schenk2004"/> | group = n }}
|-
| {{hs|09}} [[Mimas (moon)|Mimas]]
| [[Herschel (Mimantean crater)|Herschel central peak]]
| {{hs|070}}{{convert|abbr=on|7|km|mi|0}} (approx.)<ref name="Moore Schenk et al. 2004">{{cite journal| doi = 10.1016/j.icarus.2004.05.009| last1 = Moore| first1 = Jeffrey M.| last2 = Schenk| first2 = Paul M.| last3 = Bruesch| first3 = Lindsey S.| last4 = Asphaug| first4 = Erik| last5 = McKinnon| first5 = William B.| date=October 2004 | title = Large impact features on middle-sized icy satellites| journal = Icarus| volume = 171| issue = 2| pages = 421–443| url = http://planets.oma.be/ISY/pdf/article_Icy.pdf| format = PDF| bibcode = 2004Icar..171..421M| ref = {{sfnRef|Moore Schenk et al.|2004}}
}}</ref>
| {{hs|3530}} 3.5
| [[Impact crater|impact]]
| See also: [[List of largest craters in the Solar System]]
|-
| {{hs|10}} [[Dione (moon)|Dione]]
| [[List of geological features on Dione#Dorsa|Janiculum Dorsa]]
| {{hs|015}}{{convert|abbr=on|1.5|km|mi|1}}<ref name = "Hammond2013">{{Cite journal | doi = 10.1016/j.icarus.2012.12.021| title = Flexure on Dione: Investigating subsurface structure and thermal history| journal = [[Icarus (journal)|Icarus]]| volume = 223| issue = 1| pages = 418–422| date = March 2013| last1 = Hammond | first1 = N. P. | last2 = Phillips | first2 = C. B. | last3 = Nimmo | first3 = F.| last4 = Kattenhorn | first4 = S. A. | bibcode = 2013Icar..223..418H}}</ref>
| {{hs|0267}} 0.27
| [[Orogeny|tectonic]]{{refn |Was apparently formed via contraction.<ref name = "Beddingfield_2014">{{Citation
| first1 = C. B. | last1 = Beddingfield | first2 = J. P. | last2 = Emery | first3 = D. M. | last3 = Burr
| title = Testing for a Contractional Origin of Janiculum Dorsa on the Northern, Leading Hemisphere of Saturn's Moon Dione
| booktitle = 44th Lunar and Planetary Science Conference, LPI Contribution No. 1719
| pages = 1301 | publisher = [[Lunar and Planetary Institute]] | date = March 2013 | location = The Woodlands, Texas
| url = http://adsabs.harvard.edu/abs/2013LPI....44.1301B | accessdate = 23 December 2014 }}</ref><ref name='Sci Am 2017'>[https://www.scientificamerican.com/article/overlooked-ocean-worlds-fill-the-outer-solar-system/ Overlooked Ocean Worlds Fill the Outer Solar System]. John Wenz, ''Scientific American''. 4 October 2017.</ref> | group = n }}
| Surrounding crust depressed ca. 0.3&nbsp;km.
|-
| rowspan="2" | {{hs|11}} [[Titan (moon)|Titan]]
| [[Mithrim Montes]]
| {{hs|03337}}≤ {{convert|abbr=on|3.3|km|mi|1}}<ref name = "PIA20023">{{cite web | url = http://photojournal.jpl.nasa.gov/catalog/PIA20023 | title = PIA20023: Radar View of Titan's Tallest Mountains | date = 2016-03-24 | website = Photojournal.jpl.nasa.gov | publisher = [[Jet Propulsion Laboratory]] | access-date = 2016-03-25}}</ref>
| {{hs|013}} 0.13
| [[Orogeny|tectonic]]<ref name = "PIA20023" />
| May have formed due to global contraction<ref name = "Mitri">{{cite journal
| last = Mitri | first = G. | authorlink =
|author2=Bland,M. T. |author3=Showman, A. P. |author4=Radebaugh, J. |author5=Stiles, B. |author6=Lopes, R. M. C. |author7=Lunine, J. I. |author8= Pappalardo, R. T.
| title = Mountains on Titan: Modeling and observations
| journal = [[Journal of Geophysical Research]] | volume = 115 | issue = E10002
| pages = 1–15 | date = 2010 | url = http://www.agu.org/pubs/crossref/2010/2010JE003592.shtml
| doi = 10.1029/2010JE003592 | accessdate = 5 July 2012 |bibcode = 2010JGRE..11510002M }}</ref>
|-
| [[Doom Mons]]
| {{hs|0145}}{{convert|abbr=on|1.45|km|mi|2}}<ref name = "Lopes_2013">{{cite journal
| last = Lopes | first = R. M. C. | authorlink = Rosaly Lopes-Gautier
| author2 = Kirk, R. L. | author3 = Mitchell, K. L. | author4 = LeGall, A.
| author5 = Barnes, J. W. | author6 = Hayes, A. | author7 = Kargel, J.
| author8 = Wye, L. | author9 = Radebaugh, J. | author10 = Stofan, E. R.
| author11 = Janssen, M. A. | author12 = Neish, C. D. | author13 = Wall, S. D.
| author14 = Wood, C. A. | author15 = Lunine, J. I. | author16 = Malaska, M. J.
| title = Cryovolcanism on Titan: New results from Cassini RADAR and VIMS
| journal = Journal of Geophysical Research: Planets
| volume = 118 | issue = | pages = 1–20 | date = 19 March 2013
| url = http://onlinelibrary.wiley.com/doi/10.1002/jgre.20062/abstract
| doi = 10.1002/jgre.20062 | accessdate = 2013-04-10|bibcode = 2013JGRE..118..416L }}</ref>
| {{hs|0056}} 0.056
| [[cryovolcanic]]<ref name = "Lopes_2013"/>
| Adjacent to [[Sotra Patera]], a {{convert|abbr=on|1.7|km|mi|1}} deep collapse feature<ref name = "Lopes_2013"/>
|-
| {{hs|12}} [[Iapetus (moon)|Iapetus]]
| [[Equatorial ridge on Iapetus|equatorial ridge]]
| {{hs|200}}{{convert|abbr=on|20|km|mi|0}} (approx.)<ref name="GieseDenk2008">{{cite journal|last=Giese|first=B.|author2=Denk, T. |author3=Neukum, G. |author4=Roatsch, T. |author5=Helfenstein, P. |author6=Thomas, P. C. |author7=Turtle, E. P. |author8=McEwen, A. |author9= Porco, C. C. |title=The topography of Iapetus' leading side|journal=Icarus|volume=193|issue=2|date=2008|pages=359–371|issn=0019-1035|url= http://www.geoinf.fu-berlin.de/publications/denk/2008/GieseEtAl_IapetusTopography_Icarus_2008.pdf |doi=10.1016/j.icarus.2007.06.005|bibcode = 2008Icar..193..359G }}</ref>
| {{hs|2720}} 2.7
| uncertain{{refn |Hypotheses of origin include crustal readjustment associated with a decrease in [[Oblate spheroid|oblateness]] due to [[tidal locking]],<ref name="Porco2005">{{cite journal|last1=Porco|first1=C. C.| authorlink = Carolyn Porco
|display-authors=etal
|title=Cassini Imaging Science: Initial Results on Phoebe and Iapetus
|journal=Science|volume=307|issue=5713|date=2005|pages=1237–1242
|issn=0036-8075 |doi=10.1126/science.1107981 |pmid=15731440 |id=2005Sci...307.1237P|bibcode = 2005Sci...307.1237P }}</ref><ref name="kerr2006">{{cite journal
| last=Kerr | first=Richard A.
| date=2006-01-06 | title=How Saturn's Icy Moons Get a (Geologic) Life
| journal=Science | volume=311 | issue=5757 | pages=29
| doi=10.1126/science.311.5757.29
| url=http://www.sciencemag.org/cgi/content/summary/311/5757/29
| pmid=16400121}}</ref> and deposition of deorbiting material from a former [[planetary ring|ring]] around the moon.<ref name="Ip2006">{{cite journal|last1=Ip|first1=W.-H.|title=On a ring origin of the equatorial ridge of Iapetus|journal=Geophysical Research Letters|volume=33|issue=16|page=L16203 |date=2006 |issn=0094-8276|doi=10.1029/2005GL025386 |url=http://inms.space.swri.edu/publications/2006/Ip_2006.pdf|bibcode = 2006GeoRL..3316203I }}</ref> | group = n }}
| Individual peaks have not been measured
|-
| {{hs|13}} [[Oberon (moon)|Oberon]]
| unnamed ("limb mountain")
| {{hs|110}}{{convert|abbr=on|11|km|mi|0}} (approx.)<ref name="Moore Schenk et al. 2004"/>
| {{hs|1440}} 1.4
| [[Impact crater|impact]] (?)
| A value of 6&nbsp;km was given shortly after the ''[[Voyager 2]]'' encounter<ref name = "PMoore">{{cite journal
| last = Moore | first = P. | authorlink = Patrick Moore |author2=Henbest, N.
| title = Uranus - the View from Voyager
| journal = [[Journal of the British Astronomical Association]] | volume = 96 | issue = 3 | pages = 131–137
| date = April 1986 | url = http://articles.adsabs.harvard.edu/full/1986JBAA...96..131M | bibcode = 1986JBAA...96..131M
| accessdate = 7 July 2012}}</ref>
|-
| rowspan="3" | {{hs|14}} [[Pluto]]
| [[Piccard Mons]]{{refn |name=Pluto| group = n}}<ref name = "News2015-11-09">{{cite web
| url = http://pluto.jhuapl.edu/News-Center/News-Article.php?page=20151109
| title = At Pluto, New Horizons Finds Geology of All Ages, Possible Ice Volcanoes, Insight into Planetary Origins
| date = 2015-11-09 | website = New Horizons News Center
| publisher = The Johns Hopkins University Applied Physics Laboratory LLC
| access-date = 2015-11-09}}</ref><ref name = "Witze2015-11-09">{{cite web
| url = http://www.nature.com/news/icy-volcanoes-may-dot-pluto-s-surface-1.18756
| title = Icy volcanoes may dot Pluto's surface
| last = Witze | first = A. | date = 2015-11-09 | website = Nature News and Comment
| publisher = [[Nature Publishing Group]] | access-date = 2015-11-09}}</ref>
| {{hs|056}} ~{{convert|abbr=on|5.6|km|mi|1}}<ref name = "cryovolcano_topo"/>
| {{hs|0473}} 0.47
| [[cryovolcanic]] (?)
| ~220&nbsp;km across<ref name = "cryovolcano_topo">{{cite web
| url = http://pluto.jhuapl.edu/Multimedia/Science-Photos/image.php?page=&gallery_id=2&image_id=375
| title = Ice Volcanoes and Topography | date = 2015-11-09 | website = New Horizons Multimedia
| publisher = The Johns Hopkins University Applied Physics Laboratory LLC
| access-date = 2015-11-09}}</ref>
|-
| [[Wright Mons]]{{{refn |name=Pluto| group = n |Name not yet approved by the [[IAU]]}}<ref name = "News2015-11-09"/><ref name = "Witze2015-11-09"/>
| {{hs|040}} ~{{convert|abbr=on|4.0|km|mi|1}}<ref name = "News2015-11-09"/>
| {{hs|0330}} 0.34
| [[cryovolcanic]] (?)
| ~160&nbsp;km across;<ref name = "News2015-11-09"/> summit depression ~56&nbsp;km across<ref name = "Ice_Volcanoes2015-11-09">{{cite web
| url = http://pluto.jhuapl.edu/Multimedia/Science-Photos/image.php?page=&gallery_id=2&image_id=374
| title = Ice Volcanoes on Pluto? | date = 2015-11-09 | website = New Horizons Multimedia
| publisher = The Johns Hopkins University Applied Physics Laboratory LLC
| access-date = 2015-11-09}}</ref>
|-
| [[Tenzing Montes]]<ref name = "HandE_2015b">{{cite journal
| last1 = Hand | first1 = E. | last2 = Kerr | first2 = R.
| title = Potential geysers spotted on Pluto
| journal = Science | volume = 349 | issue = | pages =
| date = 17 July 2015 | doi = 10.1126/science.aac8875}}</ref>
| {{hs|035}} ≤ {{convert|abbr=on|3.5|km|mi|1}}<ref name="HandE_2015a">{{cite journal|last1=Hand|first1=E. | last2 = Kerr | first2 = R. |title=Pluto is alive—but where is the heat coming from?|journal=Science|date=15 July 2015|doi=10.1126/science.aac8860}}</ref>
| {{hs|0295}} 0.30
| [[tectonic]]<ref name = "HandE_2015a"/> (?)
| Composed of water ice;<ref name = "HandE_2015a"/> named after [[Tenzing Norgay]]<ref name="THT-20150719">{{cite web |last=Pokhrel |first=Rajan |title=Nepal’s mountaineering fraternity happy over Pluto mountains named after Tenzing Norgay Sherpa - Nepal's First Landmark In The Solar System |url=http://thehimalayantimes.com/latest/plutos-mountains-named-after-tenzing-norgay-sherpa |date=19 July 2015 |work=The Himalayan Times |accessdate= 19 July 2015}}</ref>
|}
 
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