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    High Inclination Sequence

    Date: 01 Jul 2004
    Satellite: Cassini
    Depicts: Sixth segment of Cassini's tour of Saturn
    Copyright: NASA

    Date: 31 August 2007 through 1 July 2008
    Orbit: 49 - 74 (end of nominal tour sequence)

    Studying Saturn at steep angles (high inclinations) is of extreme interest to scientists. Viewing Saturn's polar regions provides opportunities for studying Saturn's rings and magnetosphere. The high inclination sequence also allows for radio (from Earth), solar, and stellar occultations of Saturn, Titan, and the ring system. Such studies allow scientists to understand the nature of the material in Saturn, Titan, and the rings.

    This plot gives the polar view (top) and edge-on view (bottom). In the polar view the inner dashed circle represents the orbit of Titan and the outer dashed circle represents the orbit of Iapetus. The scales on the axes are in Saturn radii.


    Last Update: 30 Jul 2008

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=35610
    • Latest selection
    • Two of the PAHs found in Titan's atmosphere
    • The formation of aerosols in Titan's haze
    • The formation of aerosols in Titan's haze (annotated)
    • Image Hi-Res Versions
    • Hi-Res [gif]
      10.23 kb.
    • Related Images
    • Cassini Tour of Saturn
    • Saturn Orbit Insertion and Probe Release
    • Occultation Sequence
    • Petal Rotation and Magnetotail Petal
    • Titan 180 Transfer
    • Rotation / Icy Satellites
    • See also
    • Cassini Tour - Prime Mission
    • Titan Flyby 31.08.07
    • Titan Flyby 02.10.07
    • Titan Flyby 19.11.07
    • Titan Flyby 05.12.07
    • Titan Flyby 20.12.07
    • Titan Flyby 05.01.08
    • Enceladus Flyby 12.03.08
    • Titan Flyby 25.03.08
    • Titan Flyby 12.05.08
    • Titan Flyby 28.05.08

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