Saturn's fast spin determined from its gravitational field and oblateness
Ravit Helled, Eli Galanti, Yohai Kaspi

TL;DR
This paper determines Saturn's rotation period by analyzing its gravitational field and shape, providing a more accurate estimate than previous radio-based measurements, and validates the method on Jupiter.
Contribution
It introduces a novel method to estimate Saturn's rotation period using gravitational and shape data, overcoming limitations of magnetic and radio measurements.
Findings
Saturn's rotation period is 10h 32m 45s ± 46s.
The method accurately recovers Jupiter's known rotation period.
Gravitational and shape constraints can determine planetary rotation with minutes-level precision.
Abstract
The alignment of Saturn's magnetic pole with its rotation axis precludes the use of magnetic field measurements to determine its rotation period. The period was previously determined from radio measurements by the Voyager spacecraft to be 10h 39m 22.4s. When the Cassini spacecraft measured a period of 10h 47m 6s, which was additionally found to change between sequential measurements, it became clear that the radio period could not be used to determine the bulk planetary rotation period. Estimates based upon Saturn's measured wind fields have increased the uncertainty even more, giving numbers smaller than the Voyager rotation period, and at present Saturn's rotation period is thought to be between 10h 32m and 10h 47m, which is unsatisfactory for such a fundamental property. Here we report a period of 10h 32m 45s +- 46s, based upon an optimization approach using Saturn's measured…
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Taxonomy
TopicsAstro and Planetary Science · Geomagnetism and Paleomagnetism Studies · High-pressure geophysics and materials
