Jupiter and Saturn Rotation Periods
Ravit Helled, Gerald Schubert, and John D. Anderson

TL;DR
This paper estimates Jupiter and Saturn's rotation periods using dynamical height minimization and equilibrium theory, finding consistent results that support a rotation period of about 10h 32m for Saturn.
Contribution
It applies and compares different methods to determine Jupiter and Saturn's rotation periods, demonstrating the effectiveness of dynamical height minimization and equilibrium theory.
Findings
Jupiter's rotation period is approximately 9h 55m.
Saturn's rotation period is approximately 10h 32m.
Different methods yield consistent rotation periods for both planets.
Abstract
Anderson & Schubert (2007, Science,317,1384) proposed that Saturn's rotation period can be ascertained by minimizing the dynamic heights of the 100 mbar isosurface with respect to the geoid; they derived a rotation period of 10h 32m 35s. We investigate the same approach for Jupiter to see if the Jovian rotation period is predicted by minimizing the dynamical heights of its isobaric (1 bar pressure level) surface using zonal wind data. A rotation period of 9h 54m 29s is found. Further, we investigate the minimization method by fitting Pioneer and Voyager occultation radii for both Jupiter and Saturn. Rotation periods of 9h 55m 30s and 10h 32m 35s are found to minimize the dynamical heights for Jupiter and Saturn, respectively. Though there is no dynamical principle requiring the minimization of the dynamical heights of an isobaric surface, the successful application of the method to…
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Taxonomy
TopicsAstro and Planetary Science · Geomagnetism and Paleomagnetism Studies · Stellar, planetary, and galactic studies
