SETI public: Period Relation for the 2:1 resonance in the GJ876 planetary system

From: LARRY KLAES (ljk4_at_msn.com)
Date: Tue Jul 12 2005 - 13:04:36 UTC

  • Next message: Bill St.Arnaud: "RE: SETI public: Transmission: The Other Side of SETI"

    Paper: astro-ph/0507217
    Date: Fri, 8 Jul 2005 18:43:57 GMT (18kb)

    Title: Period Relation for the 2:1 resonance in the GJ876 planetary system

    Authors: Michael Nauenberg
    Comments: 5 pages 9 figures
    \\
    The recent radial velocity Keck data for GJ876 in Laughlin et al. (2005) is
    shown to be in good agreement, apart from a 6 m/s scatter, with a
    theoretical
    calculation (Nauenberg, 2002) based on orbital parameters from a fit to the
    earlier Keck data. The time variation of the periods of the inner and outer
    planets, which are locked in a near 2:1 resonance, are evaluated, and their
    mean values, Pi and Po, are shown to satisfy closely the relation
    Po/Pi=2+Po/P,
    where P is the period for the retrograde precesion of the common mean
    periastron of these planets.

    \\ ( http://arXiv.org/abs/astro-ph/0507217 , 18kb)

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    \\
    Paper: astro-ph/0504579
    replaced with revised version Fri, 8 Jul 2005 15:40:58 GMT (217kb)

    Title: System Parameters of the Transiting Extrasolar Planet HD 209458b

    Authors: Robert A. Wittenmyer, William F. Welsh, Jerome A. Orosz, A.B.
    Schultz,
    W. Kinzel, M. Kochte, F. Bruhweiler, D. Bennum, Gregory W. Henry, G.W.
    Marcy,
    D.A. Fischer, R.P. Butler, S.S. Vogt
    Comments: 30 pages, 5 figures. Accepted for publication in ApJ

    \\ ( http://arXiv.org/abs/astro-ph/0504579 , 217kb)


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