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- Tidal_heating abstract "Tidal heating (also known as tidal working) occurs through the tidal friction processes: orbital and rotational energy are dissipated as heat in the crust of the moons and planets involved. Io, a moon of Jupiter, is the most volcanically active body in the solar system, with no impact craters surviving on its surface. This is because the tidal force of Jupiter deforms Io; the eccentricity of Io's orbit (a consequence of its participation in a Laplace resonance) causes the height of Io's tidal bulge to vary significantly (by up to 100 m) over the course of an orbit; the friction from this tidal flexing then heats up its interior. A similar but weaker process is theorised to have melted the lower layers of the ice surrounding the rocky mantle of Jupiter's next large moon, Europa. Saturn's moon Enceladus is similarly thought to have a liquid water ocean beneath its icy crust. The water vapor geysers which eject material from Enceladus are thought to be powered by friction generated within this moon's shifting ice crust.The total amount of tidal heating is given bywhere is the satellite’s radius, is the mean orbital motion, is the eccentricity of the orbit, is a dimensionless dissipation factor, and is the shear modulus. The role of tidal heating is sometimes expressed by dimensionless number C equal to quotient of tidal heating and total internal heating.".
- Tidal_heating wikiPageID "5903656".
- Tidal_heating wikiPageRevisionID "572403614".
- Tidal_heating hasPhotoCollection Tidal_heating.
- Tidal_heating subject Category:Planetary_science.
- Tidal_heating subject Category:Tides.
- Tidal_heating type Abstraction100002137.
- Tidal_heating type Event100029378.
- Tidal_heating type Happening107283608.
- Tidal_heating type PeriodicEvent107296190.
- Tidal_heating type PsychologicalFeature100023100.
- Tidal_heating type Tide107402519.
- Tidal_heating type Tides.
- Tidal_heating type YagoPermanentlyLocatedEntity.
- Tidal_heating comment "Tidal heating (also known as tidal working) occurs through the tidal friction processes: orbital and rotational energy are dissipated as heat in the crust of the moons and planets involved. Io, a moon of Jupiter, is the most volcanically active body in the solar system, with no impact craters surviving on its surface.".
- Tidal_heating label "Aquecimento de maré".
- Tidal_heating label "Réchauffement par effet de marée".
- Tidal_heating label "Tidal heating".
- Tidal_heating label "潮汐加熱".
- Tidal_heating sameAs Réchauffement_par_effet_de_marée.
- Tidal_heating sameAs Aquecimento_de_maré.
- Tidal_heating sameAs m.0dlmfhk.
- Tidal_heating sameAs Q7800788.
- Tidal_heating sameAs Q7800788.
- Tidal_heating sameAs Tidal_heating.
- Tidal_heating wasDerivedFrom Tidal_heating?oldid=572403614.
- Tidal_heating isPrimaryTopicOf Tidal_heating.