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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 speed and hence a longer orbital…

Art, Earth–Moon system & Tidal deceleration

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Earth–Moon system

Edmond HalleyEclipsesEphemeris timeMean solar timeRichard Dunthorne
68 related topics

Tidal deceleration

Giant planetsPhobosSynchronous orbitRoche limitMars
31 related topics

Overview

Tidal forcesNatural satelliteMoonPlanetEarth
13 related topics

Other cases of tidal acceleration

DeimosBinary star
2 related topics

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Overview

Earth–Moon system

Other cases of tidal acceleration

Tidal deceleration

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Tidal acceleration

Nodes119
Edges118
Triples16
Avg. degree1.98
Density0.016807
Components1

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Tidal acceleration

Top relations

related to Other cases of tidal acceleration · 7
Tidal acceleration → Deimos, Earth-crossing, In, Mars's, Moreover, Most, The
is a · 2
Tidal acceleration → deceleration of the rotation of Earth, effect of the tidal forces between an orbiting natural satellite

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Important terminology

tidal earth moon orbit acceleration rotation time orbital effect system earth's satellites satellite moon's also angular energy deceleration rate period

Entity relationships Subject–Predicate–Object triples

SubjectPredicateObjectConfidenceSrc
Tidal accelerationis aeffect of the tidal forces between an orbiting natural satellite0.90text
Tidal accelerationis adeceleration of the rotation of Earth0.90text
the European Shelf around the British Islesinstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
the Patagonian Shelf off Argentinainstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
and the Bering Sea.The dissipation of energy by tidal friction averages about 3.64 terawatts of the 3.78 terawatts extractedinstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
of which 2.5 terawatts are from the principal M2 lunar componentinstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
the remainder from other componentsinstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
both lunarinstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
solar.An equilibrium tidal bulge does not really exist on Earth because the continents do not allow this mathematical solution to take placeinstance ofMost of the dissipation occurs in a turbulent bottom boundary layer in shallow seas0.80text
Tidal accelerationrelated to Other cases of tidal accelerationMost0.60section
Tidal accelerationrelated to Other cases of tidal accelerationIn0.60section
Tidal accelerationrelated to Other cases of tidal accelerationThe0.60section

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