SETI bioastro: Fw: Scientists Find That Saturn's Rotation Period Is A Puzzle

From: LARRY KLAES (ljk4_at_msn.com)
Date: Thu Jul 01 2004 - 13:57:02 PDT

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    ----- Original Message -----
    From: NASA Jet Propulsion Laboratory<mailto:info_at_jpl.nasa.gov>
    To: ljk4_at_msn.com<mailto:ljk4_at_msn.com>
    Sent: Monday, June 28, 2004 7:18 PM
    Subject: Scientists Find That Saturn's Rotation Period Is A Puzzle

    MEDIA RELATIONS OFFICE
    JET PROPULSION LABORATORY
    CALIFORNIA INSTITUTE OF TECHNOLOGY
    NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
    PASADENA, CALIFORNIA 91109. TELEPHONE (818) 354-5011
    http://www.jpl.nasa.gov>

    Carolina Martinez (818) 354-9382
    Jet Propulsion Laboratory, Pasadena, Calif.

    Gary Galluzzo (319) 384-0009
    University of Iowa, Iowa City

    News Release: 2004-164 June 28, 2004

    Scientists Find That Saturn's Rotation Period Is A Puzzle

    On approach to Saturn, data obtained by the Cassini spacecraft are
    already posing a puzzling question: How long is the day on Saturn?

    Cassini took readings of the day-length indicator regarded as most
    reliable, the rhythm of natural radio signals from the planet. The
    results give 10 hours, 45 minutes, 45 seconds (plus or minus 36
    seconds) as the length of time it takes Saturn to complete each
    rotation. Here's the puzzle: That is about 6 minutes, or one percent,
    longer than the radio rotational period measured by the Voyager 1 and
    Voyager 2 spacecraft, which flew by Saturn in 1980 and 1981.

    Cassini scientists are not questioning Voyager's careful measurements.
    And they definitely do not think the whole planet of Saturn is
    actually rotating that much slower than it did two decades ago.
    Instead, they are looking for an explanation based on some variability
    in how the rotation deep inside Saturn drives the radio pulse.

    The radio sounds of Saturn's rotation, which are also the first sounds
    from Saturn studied by Cassini, are like a heartbeat and can be heard
    by visiting
    http://www.jpl.nasa.gov/videos/cassini/0604/> and
    http://www-pw.physics.uiowa.edu/space-audio>

    "The rotational modulation of radio emissions from distant
    astronomical objects has long been used to provide very accurate
    measurements of their rotation period," said Dr. Don Gurnett,
    principal investigator for the Cassini Radio and Plasma Wave Science
    instrument, University of Iowa, Iowa City. "The technique is
    particularly useful for the giant gas planets, such as Jupiter and
    Saturn, which have no surfaces and are covered by clouds that make
    direct visual measurements impossible."

    The first hint of something strange about that type of measurement at
    Saturn was in 1997, when a researcher from Observatoire de Paris
    reported that Saturn's radio rotation period differed substantially
    from Voyager.

    Dr. Michael D. Desch, Cassini Radio Plasma Wave Science team member,
    and scientist at NASA's Goddard Space Flight Center in Greenbelt, Md.,
    has analyzed Saturn radio data collected by Cassini from April 29,
    2003, to June 10, 2004. "We all agree that the radio rotation period
    of Saturn is longer today than it was in during the Voyager flyby in
    1980," he said.

    Gurnett said, "Although Saturn's radio rotation period has clearly
    shifted substantially since the Voyager measurements, I don't think
    any of us could conceive of any process that would cause the rotation
    of the entire planet to actually slow down. So it appears that there
    is some kind of slippage between the deep interior of the planet and
    the magnetic field, which controls the charged particles responsible
    for the radio emission." He suggests the solution may be tied to the
    fact that Saturn's rotational axis is nearly identical to its magnetic
    axis. Jupiter, with a more substantial difference between its
    magnetic axis and its rotational axis, shows no comparable
    irregularities in its radio rotation period.

    "This finding is very significant. It demonstrates that the idea of a
    rigidly rotating magnetic field is wrong," said Dr. Alex Dessler, a
    senior research scientist at the University of Arizona, Tucson. In
    that way, the magnetic fields of gas giant planets may resemble that
    of the Sun. The Sun's magnetic field does not rotate uniformly.
    Instead, its rotation period varies with latitude. "Saturn's magnetic
    field has more in common with the Sun than the Earth. The measurement
    can be interpreted as showing that the part of Saturn's magnetic field
    that controls the radio emissions has moved to a higher latitude
    during the last two decades," said Dressler.

    "I think we will be able to unravel the puzzle, but it's going to take
    some time," said Gurnett. "With Cassini in orbit around Saturn for
    four years or more, we will be in an excellent position to monitor
    long-term variations in the radio period, as well as investigate the
    rotational period using other techniques."

    Cassini, carrying 12 scientific instruments, is just two days from its
    planetary rendezvous with Saturn. On June 30 it will become the first
    spacecraft to orbit Saturn, when it begins a four-year study of the
    planet, its rings and its 31 known moons. The spacecraft recently flew
    past Saturn's cratered moon Phoebe, where it captured spectacular
    images as well as data on its mass and composition.

    The Cassini-Huygens mission is a cooperative project of NASA, the
    European Space Agency and the Italian Space Agency. The Jet Propulsion
    Laboratory, a division of the California Institute of Technology in
    Pasadena, manages the Cassini-Huygens mission for NASA's Office of
    Space Science, Washington, D.C. JPL designed, developed and assembled
    the Cassini orbiter.
    For the latest images and more information about the Cassini-Huygens
    mission, visit
    http://www.nasa.gov/cassini>

    -end-


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