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    ESA > Space in Images > 2012 > 06 > Titan’s tides raised by Saturn

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    Titan’s tides raised by Saturn

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    • Title Titan’s tides raised by Saturn
    • Released 28/06/2012 10:26 am
    • Copyright NASA/JPL
    • Description

      Titan orbits Saturn on an elliptical path once every 16 days.
      The shape of the moon changes along its orbit because of the varying tidal
      pull from Saturn such that it is stretched into a rugby-ball shape at its
      closest point to the gas giant and is more spherical at its most distant
      point. The change in shape causes a redistribution of mass in the moon and
      therefore a change in the gravity field, which is measured by Cassini in the
      form of the change in acceleration of the spacecraft as tracked by microwave
      radio links with the ground antennas of NASA’s Deep Space Network. The
      measurements were taken along different points of Titan’s orbit and
      correspond to a tidal deformation of about 10 m. Since the amplitude of solid
      tides depends on the overall rigidity of the body’s interior and on the
      strength of the gravitational pull of nearby objects, Titan must have a
      liquid ocean at depth to accommodate this amount of tidal deformation.


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