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| | Tectonic Processes on Europa: |
 | | Together these considerations provide a model in which currently observed cracks were produced as Europa rotated through the last several tens of degrees relative to the direction of Jupiter, with crack patterns affected by stress due to both non-synchronous rotation and diurnal tides, possibly during the past several hundred thousand years. |
 | | For a satellite on an eccentric orbit, even if it rotates synchronously, the magnitude and orientation of the tidal distortion due to the planet changes with a period equal to the orbital period. |
 | | For any very small angle of rotation, the pattern is similar, with amplitudes approximately proportional to the angle, and with symmetry offset from the cardinal longitudes (0o, 90o, 180o, 270o) by 45o. |
| pirlwww.lpl.arizona.edu /HIIPS/Publications/greenberg_tectonics (9541 words) |
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