4.8 Article

Saturn's rotation period from its atmospheric planetary-wave configuration

Journal

NATURE
Volume 460, Issue 7255, Pages 608-610

Publisher

NATURE PUBLISHING GROUP
DOI: 10.1038/nature08194

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Funding

  1. UK Science and Technology Facilities Council
  2. NASA's Planetary Atmospheres and Outer Planet Research Programs

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The rotation period of a gas giant's magnetic field (called the System III reference frame) is commonly used to infer its bulk rotation(1). Saturn's dipole magnetic field is not tilted relative to its rotation axis (unlike Jupiter, Uranus and Neptune), so the surrogate measure of its long-wavelength (kilometric) radiation is currently used to fix the System III rotation period(2). The period as measured now by the Cassini spacecraft is up to similar to 7 min longer(3) than the value of 10 h 39 min 24 s measured 28 years ago by Voyager(2). Here we report a determination of Saturn's rotation period based on an analysis of potential vorticity. The resulting reference frame (which we call System IIIw) rotates with a period of 10 h 34 min 13 +/- 20 s. This shifted reference frame is consistent with a pattern of alternating jets on Saturn that is more symmetrical between eastward and westward flow. This suggests that Saturn's winds are much more like those of Jupiter than hitherto believed(4).

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