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  2. Tidal heating - Wikipedia

    en.wikipedia.org/wiki/Tidal_heating

    Tidal heating (also known as tidal working or tidal flexing) occurs through the tidal friction processes: orbital and rotational energy is dissipated as heat in either (or both) the surface ocean or interior of a planet or satellite. When an object is in an elliptical orbit, the tidal forces acting on it are stronger near periapsis than near ...

  3. Tidal heating of Io - Wikipedia

    en.wikipedia.org/wiki/Tidal_heating_of_Io

    Tidal heating of Io (also known as tidal working) occurs through the tidal friction processes between Jupiter and its moon. Orbital and rotational energy are dissipated as heat in the crust of the moon. Io has a similar mass and size as the Moon, but Io is the most geologically active body in the Solar System. This is caused by the heating ...

  4. Tidal acceleration - Wikipedia

    en.wikipedia.org/wiki/Tidal_acceleration

    Tidal acceleration is an effect of the tidal forces between an orbiting natural satellite (e.g. the Moon) and the primary planet that it orbits (e.g. Earth). The acceleration causes a gradual recession of a satellite in a prograde orbit (satellite moving to a higher orbit, away from the primary body, with a lower orbital velocity and hence a ...

  5. Dynamo theory - Wikipedia

    en.wikipedia.org/wiki/Dynamo_theory

    This is known as tidal heating, and it helps keep the interior in a liquid state. A liquid interior that can conduct electricity is required to produce a dynamo. Saturn's Enceladus and Jupiter's Io have enough tidal heating to liquify their inner cores, but they may not create a dynamo because they cannot conduct electricity.

  6. Tidal locking - Wikipedia

    en.wikipedia.org/wiki/Tidal_locking

    Due to tidal locking, the inhabitants of the central body will never be able to see the satellite's green area. All twenty known moons in the Solar System that are large enough to be round are tidally locked with their primaries, because they orbit very closely and tidal force increases rapidly (as a cubic function) with decreasing distance. [16]

  7. Volcanism - Wikipedia

    en.wikipedia.org/wiki/Volcanism

    Volcanism on outer solar system moons is powered mainly by tidal heating. [1] Tidal heating caused by the deformation of a body's shape due to mutual gravitational attraction, which generates heat. Earth experiences tidal heating from the Moon, deforming by up to 1 metre (3 feet), but this does not make up a major portion of Earth's total heat. [4]

  8. As erosion and floods swallow buildings, Washington's ... - AOL

    www.aol.com/erosion-floods-swallow-buildings...

    North Cove is in the northwest corner of Washington's Pacific County, where sea level projections show a 96% chance that at least one coastal flood reaching five feet above the high tide line will ...

  9. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    This would have led to orbital eccentricity and tidal heating that may have warmed Tethys' interior enough to form a subsurface ocean. Subsequent freezing of the ocean after the moons escaped from the resonance may have generated the extensional stresses that created the enormous graben system of Ithaca Chasma on Tethys.