Diferencies ente revisiones de «Ganimedes (lluna)»
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[[File:Ganymede diagram.svg|thumb|400px|right|Representación artística de la estructura interna de Ganimedes. Les capes tán representaes a escala.]]
Yá na década de 1970 los científicos de la [[NASA]] entamaron a sospechar la esistencia en Ganimedes d'un océanu perprofundu encerráu ente dos capas de xelu, una superficial y otra que envuelve, en contautu directu con elli, el mantu rocosu<ref name="Showman1999" /><ref name="clubsandwich 2014" />{<ref name="Sohl2002" /><ref name="Freeman2006">{{cite journal |last=Freeman |first=J. |title=Non-Newtonian stagnant lid convection and the thermal evolution of Ganymede and Callisto |journal=Planetary and Space Science |date=2006 |volume=54 |issue=1 |pages=2–14 |doi=10.1016/j.pss.2005.10.003 |url=http://bowfell.geol.ucl.ac.uk/~lidunka/EPSS-papers/pete2.pdf |archiveurl=https://web.archive.org/web/20070824155106/http://bowfell.geol.ucl.ac.uk/~lidunka/EPSS-papers/pete2.pdf |archivedate=2007-08-24 |format=PDF |bibcode=2006P&SS...54....2F }}</ref><ref name="amount of water in ocean">{{cite web | url=http://earthsky.org/space/underground-ocean-on-jupiters-largest-moon | title=Underground ocean on Jupiter's largest moon | publisher=EarthSky | date=March 15, 2015 | accessdate=17 de febreru de 2017 }}</ref>. Na década de 1990 la misión ''Galileo'' sobrevoló'l satélite, confirmando la esistencia d'esti océanu soterrañu. Un análisis asoleyáu en [[2014]], que tien en cuenta la termodinámica de les mases d'agua y los efectos del sal, suxere que Ganimedes podría tener delles capes oceániques d'agua líquido separtaes por capes de xelu, cola capa más profunda en contautu directu col mantu rocosu<ref name="clubsandwich 2014" /><ref name="Vance">{{cite journal |title=Ganymede's internal structure including thermodynamics of magnesium sulfate oceans in contact with ice |journal=Planetary and Space Science |date=12 April 2014 |last=Vance |first=Steve |last2=Bouffard |first2=Mathieu |last3=Choukroun |first3=Mathieu |last4=Sotina |first4=Christophe |doi=10.1016/j.pss.2014.03.011 |url=http://www.sciencedirect.com/science/article/pii/S0032063314000695 |accessdate=17 de febreru de 2017 |bibcode = 2014P&SS...96...62V |volume=96 |pages=62–70}}</ref>
<ref name="NASA-20140501c">{{cite web |author=Staff |title=
Hai delles especulaciones, nel ámbitu científicu, sobre l'habitabilidá potencial del océanu ganimedín<ref name="amount of water in ocean" /><ref name="subsurface ocean found">{{cite web | url=http://www.independent.co.uk/news/science/ganymede-oceans-on-jupiters-moon-could-have-been-home-to-alien-life-10106286.html | title=Ganymede oceans on Jupiter's moon could have been home to alien life | publisher=The Independent | date=March 13, 2015 | accessdate=17 de febreru de 2017 | author=Griffin, Andrew}}</ref>.
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