• → European Space Agency

    • About Science & Technology

    • For Public

    • For Educators

    • ESA

    • Science & Technology

    • Cassini-Huygens

    • Missions
    • Show All Missions
    • Mission Home
    • Summary
    • Fact Sheet
    • Objectives
    • Mission Team
    • Orbit View
    • Science…

      • Saturn
      • Rings
      • Titan
      • Moons
      • Magnetosphere
    • Huygens Probe
    • Huygens
    • Instruments
    • Engineering
    • Cassini Orbiter
    • 3D Model
    • Instruments
    • Engineering
    • Mission Operations
    • Launch Vehicle
    • Launch Information
    • Approach and Arrival
    • Getting to Saturn
    • Huygens Probe Separation
    • Titan Surface Landing
    • Flybys
    • Science Operations
    • Data Archive
    • Resources
    • News Archive
    • Multimedia Gallery
    • Publication Archive
    • Calendar of Events
    • Services
    • Contact Us
    • Subscribe
    • Terms and Conditions
    • Bookmark and Share

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

    Publication date: 30 Jul 2009

    Authors: Read, P.L. et al.

    Journal: Nature
    Volume: 460
    Issue: 7255
    Page: 608-610
    Year: 2009

    Copyright: Nature Publishing Group

    The rotation period of a gas giant's magnetic field (called the System III reference frame) is commonly used to infer its bulk rotation. 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. The period as measured now by the Cassini spacecraft is up to ~7 min longer than the value of 10 h 39 min 24 s measured 28 years ago by Voyager. 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.

    Link to Publication

    Last Update: 30 Jul 2009

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=45384

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Livestream
    • Subscribe
    • App Store
    • ESA Science Twitter

    Follow ESA science

    • Copyright 2000 - 2013 © European Space Agency. All rights reserved.

    • Terms and Conditions