Herdersmaan: Verskil tussen weergawes
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k Robot: standardiseer verwysingsjablone en voeg argiefskakels in. |
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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>{{
[[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>
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