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Geophysical implications of the long-wavelength topography of the Saturnian satellites

Geophysical implications of the long-wavelength topography of the Saturnian satellites

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_903594802

Geophysical implications of the long-wavelength topography of the Saturnian satellites

About this item

Full title

Geophysical implications of the long-wavelength topography of the Saturnian satellites

Publisher

Washington: Blackwell Publishing Ltd

Journal title

Journal of Geophysical Research, 2011-11, Vol.116 (E11), p.n/a, Article E11001

Language

English

Formats

Publication information

Publisher

Washington: Blackwell Publishing Ltd

More information

Scope and Contents

Contents

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...

Alternative Titles

Full title

Geophysical implications of the long-wavelength topography of the Saturnian satellites

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_903594802

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_903594802

Other Identifiers

ISSN

0148-0227,2169-9097

E-ISSN

2156-2202,2169-9100

DOI

10.1029/2011JE003835

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