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Cassini Radio Science

  • Chapter
The Cassini-Huygens Mission

Abstract

Cassini radio science investigations will be conducted both during the cruise (gravitational wave and conjunction experiments) and the Saturnian tour of the mission (atmospheric and ionospheric occultations, ring occultations, determinations of masses and gravity fields). New technologies in the construction of the instrument, which consists of a portion on-board the spacecraft and another portion on the ground, including the use of the Ka-band signal in addition to that of the S- and X-bands, open opportunities for important discoveries in each of the above scientific areas, due to increased accuracy, resolution, sensitivity, and dynamic range.

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  1. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA

    J. D. Anderson, J. W. Armstrong, S. W. Asmar, C. L. Hamilton, N. J. Rappaport & H. D. Wahlquist

  2. Istituto di Radioastronomia CNR, Via Gobetti 101, 1-40129, Bologna, Italy

    R. Ambrosini

  3. NASA-Goddard Space Flight Center, Greenbelt, MD, 20771, USA

    F. M. Flasar

  4. Wellesley College, Wellesley, MA, 02481, USA

    R. G. French

  5. Università di Roma ‘La Sapienza’, Via Eudossiana 18, I-00184, Roma, Italy

    L. Iess

  6. San Jose State University, One Washington Square, San Jose, CA, 95192, USA

    E. A. Marouf

  7. University of Michigan, 2455 Hayward Avenue, Ann Arbor, MI, 48109, USA

    A. F. Nagy

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    Christopher T. Russell

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Kliore, A.J. et al. (2004). Cassini Radio Science. In: Russell, C.T. (eds) The Cassini-Huygens Mission. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3874-7_1

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