Saturnus se natuurlike satelliete: Verskil tussen weergawes

'''Saturnus se natuurlike satelliete''' is talryk en uiteenlopend.<ref name="NYT-20151218-jc">{{cite news |last=Corum |first=Jonathan |title=Mapping Saturn’s Moons |url=https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html |date=18 Desember 2015 |work=New York Times |access-date=18 Desember 2015 |language=en |archive-url=https://web.archive.org/web/20200520124847/https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html |archive-date=20 Mei 2020 |url-status=live |df=dmy-all}}</ref> Hulle wissel van klein maantjies van minder as ’n [[kilometer]] breed tot die enorme [[Titaan (maan)|Titaan]], wat groter as die planeet [[Mercurius]] is. [[Saturnus]] het 82 [[Natuurlike satelliet|mane]] met bevestigde [[Wentelbaan|wentelbane]],<ref>https://www.bbc.co.uk/news/science-environment-49962134</ref> waarvan 53 name en net 13 ’n deursnee van meer as 50&nbsp;km het, sowel as [[Saturnus se ringe|ringe]] met komplekse wentelbewegings van hulle eie.<ref name="Saturn62">{{cite web |url=http://ssd.jpl.nasa.gov/?sat_discovery |title=Solar System Exploration Planets Saturn: Moons: S/2009 S1 |publisher=Nasa |access-date=17 Januarie 2010 |language=en |archive-url=https://web.archive.org/web/20200523050403/https://ssd.jpl.nasa.gov/?sat_discovery |archive-date=23 Mei 2020 |url-status=live |df=dmy-all}}</ref><ref name=shep-main>{{cite web |url=http://www.dtm.ciw.edu/users/sheppard/satellites/ |title=The Giant Planet Satellite and Moon Page |author=Sheppard, Scott S. |publisher=Departament of Terrestrial Magnetism at Carniege Institution for science |access-date=28 Augustus 2008 |language=en |archive-url=https://web.archive.org/web/20130922232711/http://www.dtm.ciw.edu/users/sheppard/satellites/ |archive-date=22 September 2013 |url-status=live |df=dmy-all}}</ref><ref name="IAUC2009b">{{cite journal|author1=Porco, C. |author2=the Cassini Imaging Team |lastauthoramp=yes | title= S/2009 S1| journal=IAU Circular| volume= 9091| url= http://ciclops.org/view_popup.php?id=5926&js=1|date=2 November 2009}}</ref> Sewe van Saturnus se mane is groot genoeg om die vorm van ’n [[ellips]]oïed te hê, hoewel net twee, Titaan en [[Rea (maan)|Rea]], tans in [[hidrostatiese ewewig]] is.