Kronoseismology VI: Reading the recent history of Saturn's gravity field in its rings
M.M. Hedman, P.D. Nicholson, M. El Moutamid, S. Smotherman

TL;DR
This study uses wavelet analysis of Cassini data to uncover transient and persistent gravitational anomalies in Saturn's interior, revealing their evolution over decades and their influence on the planet's gravity field.
Contribution
It introduces a novel application of wavelet-based analysis combined with density wave theory to map and track Saturn's gravitational anomalies over time.
Findings
Identified transient gravitational anomalies with lifespans of a few years.
Detected a persistent anomaly with a steadily increasing rotation rate from 1970 to 2010.
Discovered two gravity field asymmetries with different azimuthal wavenumbers and rotation rates.
Abstract
Saturn's C ring contains multiple structures that appear to be density waves driven by time-variable anomalies in the planet's gravitational field. Semi-empirical extensions of density wave theory enable the observed wave properties to be translated into information about how the pattern speeds and amplitudes of these gravitational anomalies have changed over time. Combining these theoretical tools with wavelet-based analyses of data obtained by the Visual and Infrared Mapping Spectrometer (VIMS) onboard the Cassini spacecraft reveals a suite of structures in Saturn's gravity field with azimuthal wavenumber 3, rotation rates between 804 degrees/day and 842 degrees/day and local gravitational potential amplitudes between 30 and 150 cm^2/s^2. Some of these anomalies are transient, appearing and disappearing over the course of a few Earth years, while others persist for decades. Most of…
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Taxonomy
TopicsAstro and Planetary Science · Geomagnetism and Paleomagnetism Studies · Stellar, planetary, and galactic studies
