ผลต่างระหว่างรุ่นของ "ผู้ใช้:EZBELLA/กระบะทราย6"

| Formed by the [[Caloris Basin|Caloris impact]]

|-

| [[Skadi Mons]]

| {{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>

| Highest volcano on Venus

|-

| [[Mauna Kea]] and [[Mauna Loa]]<!--they are effectively the same height at this scale-->

| {{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>

|{{convert|abbr=on|2.8|to|3.2|km|mi|1}} -->

|-

| [[Mons Huygens]]

| {{convert|abbr=on|5.5|km|mi|1}}<ref name="price"/><ref name="moore"/>

| Largest volcanic construct on the Moon<ref name="laps07"/>

|-

| [[Olympus Mons]]

| {{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" />

| 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>

|-

| [[Rheasilvia|Rheasilvia central peak]]

|{{convert|abbr=on|22|km|mi|0}}<ref name="Vega">{{cite web

| Almost {{convert|200|km|mi|abbr=on}} wide. See also: [[List of largest craters in the Solar System]]

|-

| [[Ahuna Mons]]

| {{convert|abbr=on|4|km|mi|1}}<ref name = "Ceres">{{cite web

| Isolated steep-sided dome in relatively smooth area; max. height of ~ 5&nbsp;km on steepest side; roughly [[Antipodes|antipodal]] to [[Kerwan (crater)|largest impact basin on Ceres]]

|-

| [[Boösaule Montes]] "South"<ref name = "Boösaule Montes">{{cite web

| last = Perry | first = Jason | title = Boösaule Montes

| 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 }}

|-

| [[Herschel (Mimantean crater)|Herschel central peak]]

| {{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}}

| See also: [[List of largest craters in the Solar System]]

|-

| [[List of geological features on Dione#Dorsa|Janiculum Dorsa]]

| {{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>

| Surrounding crust depressed ca. 0.3&nbsp;km.

|-

| [[Mithrim Montes]]

| ≤ {{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>

| Adjacent to [[Sotra Patera]], a {{convert|abbr=on|1.7|km|mi|1}} deep collapse feature<ref name = "Lopes_2013"/>

|-

| [[Equatorial ridge on Iapetus|equatorial ridge]]

| {{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>

| Individual peaks have not been measured

|-

| unnamed ("limb mountain")

| {{convert|abbr=on|11|km|mi|0}} (approx.)<ref name="Moore Schenk et al. 2004"/>

| accessdate = 7 July 2012}}</ref>

|-

| [[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

| [[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>

|}

 

==Gallery==