The Legacy of Galileo - Keck Institute for Space Studies - Caltech
The Legacy of Galileo - Keck Institute for Space Studies - Caltech
The Legacy of Galileo - Keck Institute for Space Studies - Caltech
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Challenging the Paradigm: <strong>The</strong> <strong>Legacy</strong> <strong>of</strong> <strong>Galileo</strong><br />
(Figure 10). Gravity data taken during the close flybys also indicated a low density (i.e., ~1000<br />
kg/m-3) layer about 100 km deep overlying a denser rock and iron interior. <strong>The</strong>se<br />
observations were all consistent with models showing that a liquid water ocean, with a<br />
volume twice that <strong>of</strong> all Earth’s oceans, could be maintained under an icy crust by tidal<br />
dissipation.<br />
Figure 10: Europa’s blocks <strong>of</strong> ice.<br />
Crucial evidence <strong>for</strong> a subsurface ocean at not only Europa, but also Ganymede and Callisto<br />
came from magnetic field data. Only Ganymede, as described earlier, exhibits a strong, fixed,<br />
dipole-like magnetic field indicative <strong>of</strong> an internal dynamo. However, significant magnetic<br />
deflections were observed during close flybys <strong>of</strong> each <strong>of</strong> the icy satellites, with the pattern <strong>of</strong><br />
the deflection changing from encounter to encounter. Correlating these magnetic<br />
perturbations with the direction and timing <strong>of</strong> Jupiter’s magnetic field, the magnetometer<br />
investigators found that the perturbations exactly matched calculations <strong>for</strong> an induced<br />
magnetic field produced by changes in Jupiter’s field as the planet rotates. <strong>The</strong> satellites are<br />
embedded in the magnetosphere, and Jupiter’s dipole field is tilted about ten degrees to the<br />
planet’s rotation axis. Thus, the magnetic field seen by each satellite rocks back and <strong>for</strong>th,<br />
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