Herdersmaan: Verskil tussen weergawes

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k Robot: standardiseer verwysingsjablone en voeg argiefskakels in.
Lyn 9:
Twee van [[Jupiter]] se klein binneste mane, [[Metis (maan)|Metis]] en [[Adrastea (maan)|Adrastea]], lê binne [[Jupiter se ringe]] en ook binne die planeet se [[Rochelimiet]].<ref>{{Cite book|title=Introduction to Planetary Science: The Geological Perspective|last=Faure|first=Gunter|last2=Mensing|first2=Teresa|publisher=Springer|year=2007|isbn=978-1-4020-5233-0|location=|pages=}}</ref> Dit is moontlik dat dié ringe saamgestel is uit materiaal wat van dié twee liggame getrek word deur Jupiter se getykragte, aangehelp deur botsings van ringmateriaal teen hul oppervlakke.
 
[[Saturnus]] se ingewikkelde [[Saturnus se ringe|ringstelsel]] het verskeie sulke satelliete. Dit sluit in [[Prometheus (maan)|Prometheus]] (F-ring),<ref>{{Citecite web |url=http://www.planetary.org/blogs/emily-lakdawalla/2014/07010001-ringmoons-shepherds.html |title=On the masses and motions of mini-moons: Pandora's not a |website=www.planetary.org |access-date=14 Junie 2016 |language=en |archive-06url=https://web.archive.org/web/20200127203502/https://www.planetary.org/blogs/emily-14lakdawalla/2014/07010001-ringmoons-shepherds.html |archive-date=27 Januarie 2020 |url-status=live|df=dmy-all}}</ref> [[Daphnis (maan)|Daphnis]] (Keeler-gaping),<ref>{{Citecite web |url=http://www.nasa.gov/mission_pages/cassini/media/cassini-051005.html |title=NASA - Cassini Finds New Saturn Moon That Makes Waves |website=www.nasa.gov |access-date=14 Junie 2016 |language=en |accessarchive-url=https://web.archive.org/web/20170513161508/https://www.nasa.gov/mission_pages/cassini/media/cassini-051005.html |archive-date=201613 Mei 2017 |url-06status=live|df=dmy-14all}}</ref> [[Pan (maan)|Pan]] (Encke-gaping),<ref>{{Cite journal|last=Showalter|first=Mark R.|date=1991-06-27|title=Visual detection of 1981S13, Saturn's eighteenth satellite, and its role in the Encke gap|url=http://www.nature.com/nature/journal/v351/n6329/abs/351709a0.html|journal=Nature|language=en|volume=351|issue=6329|pages=709–713|doi=10.1038/351709a0|bibcode = 1991Natur.351..709S }}</ref> [[Janus (maan)|Janus]] en [[Epimetheus (maan)|Epimetheus]] (albei A-ring).<ref>{{Cite journal|last=Moutamid|first=Maryame El|last2=Nicholson|first2=Philip D.|last3=French|first3=Richard G.|last4=Tiscareno|first4=Matthew S.|last5=Murray|first5=Carl D.|last6=Evans|first6=Michael W.|last7=French|first7=Colleen McGhee|last8=Hedman|first8=Matthew M.|last9=Burns|first9=Joseph A.|date=2015-10-01|title=How Janus' Orbital Swap Affects the Edge of Saturn's A Ring?|arxiv=1510.00434|bibcode = 2016Icar..279..125E |doi = 10.1016/j.icarus.2015.10.025 }}</ref>
 
[[Uranus]] het ook herdersmane in sy ε-ring, [[Cordelia (maan)|Cordelia]] en [[Ophelia (maan)|Ophelia]]. Hulle is onderskeidelik binneste en buitenste herdersmane.<ref>{{Cite journal|last=Esposito|first=Larry W.|date=2002-01-01|title=Planetary rings|url=http://stacks.iop.org/0034-4885/65/i=12/a=201|journal=Reports on Progress in Physics|language=en|volume=65|issue=12|pages=1741–1783|doi=10.1088/0034-4885/65/12/201|issn=0034-4885|bibcode = 2002RPPh...65.1741E }}</ref> Albei is binne Uranus se sinchroniese wentelradius en hul wentelbane neem dus stadig af weens getyvertraging.<ref>{{Cite journal|last=Karkoschka|first=Erich|date=2001-05-01|title=Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites|url=http://www.sciencedirect.com/science/article/pii/S0019103501965972|journal=Icarus|volume=151|issue=1|pages=69–77|doi=10.1006/icar.2001.6597|bibcode=2001Icar..151...69K}}</ref>