Geophysical implications of the long-wavelength topography of the Saturnian satellites
Geophysical implications of the long-wavelength topography of the Saturnian satellites
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Washington: Blackwell Publishing Ltd
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English
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Washington: Blackwell Publishing Ltd
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We use limb profiles to quantify the long‐wavelength topography of the Saturnian satellites. The degree 2 shapes of Mimas, Enceladus, and Tethys are not consistent with hydrostatic equilibrium. We derive 2‐D topographic maps out to spherical harmonic degree 8. There is a good correlation with topography derived from stereo techniques. If uncompensa...
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Geophysical implications of the long-wavelength topography of the Saturnian satellites
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TN_cdi_proquest_journals_903594802
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_903594802
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ISSN
0148-0227,2169-9097
E-ISSN
2156-2202,2169-9100
DOI
10.1029/2011JE003835