SETI bioastro: Observations of Extrasolar Planets During the non-Cryogenic Spitzer Space Telesc

From: LARRY KLAES (ljk4_at_msn.com)
Date: Wed Oct 24 2007 - 11:00:41 PDT

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    Observations of Extrasolar Planets During the non-Cryogenic Spitzer Space
    Telescope Mission

    Authors: Drake Deming, Eric Agol, David Charbonneau, Nicolas Cowan, Heather
    Knutson, Massimo Marengo

    (Submitted on 22 Oct 2007)

    Abstract: Precision infrared photometry from Spitzer has enabled the first
    direct studies of light from extrasolar planets, via observations at
    secondary eclipse in transiting systems. Current Spitzer results include the
    first longitudinal temperature map of an extrasolar planet, and the first
    spectra of their atmospheres. Spitzer has also measured a temperature and
    precise radius for the first transiting Neptune-sized exoplanet, and is
    beginning to make precise transit timing measurements to infer the existence
    of unseen low mass planets. The lack of stellar limb darkening in the
    infrared facilitates precise radius and transit timing measurements of
    transiting planets. Warm Spitzer will be capable of a precise radius
    measurement for Earth-sized planets transiting nearby M-dwarfs, thereby
    constraining their bulk composition. It will continue to measure thermal
    emission at secondary eclipse for transiting hot Jupiters, and be able to
    distinguish between planets having broad band emission versus absorption
    spectra. It will also be able to measure the orbital phase variation of
    thermal emission for close-in planets, even non-transiting planets, and
    these measurements will be of special interest for planets in eccentric
    orbits. Warm Spitzer will be a significant complement to Kepler,
    particularly as regards transit timing in the Kepler field. In addition to
    studying close-in planets, Warm Spitzer will have significant application in
    sensitive imaging searches for young planets at relatively large angular
    separations from their parent stars.

    Comments: 12 pages, 7 figures, to appear in “Science Opportunities for the
    Warm Spitzer Mission”

    Subjects: Astrophysics (astro-ph)

    Cite as: arXiv:0710.4145v1 [astro-ph]

    Submission history

    From: Drake Deming [view email]

    [v1] Mon, 22 Oct 2007 20:34:53 GMT (310kb)

    http://arxiv.org/abs/0710.4145


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