SETI public: Atmospheric Biomarkers and their Evolution over Geological Timescales

From: LARRY KLAES (ljk4_at_msn.com)
Date: Mon Dec 05 2005 - 08:29:38 PST

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    Paper: astro-ph/0512053

    Date: Fri, 2 Dec 2005 02:47:13 GMT (391kb)

    Title: Atmospheric Biomarkers and their Evolution over Geological Timescales

    Authors: L. Kaltenegger, K. Jucks, W.Traub

    Comments: for high resolution images see

    http://cfa-www.harvard.edu/~lkaltenegger

    Journal-ref: CUP, IAUC 200 proceedings, 2005
    \\
    The search for life on extrasolar planets is based on the assumption that
    one
    can screen extrasolar planets for habitability spectroscopically. The first
    space born instruments able to detect as well as characterize extrasolar
    planets, Darwin and terrestrial planet finder (TPF-I and TPF-C) are
    scheduled
    to launch before the end of the next decade. The composition of the
    planetary
    surface, atmosphere, and its temperature-pressure profile influence a
    detectable spectroscopic signal considerably.

    For future space-based missions it will be crucial to know this influence to
    interpret the observed signals and detect signatures of life in remotely
    observed atmospheres.

    We give an overview of biomarkers in the visible and IR range, corresponding
    to the TPF-C and TPF-I/DARWIN concepts, respectively. We also give an
    overview of the evolution of biomarkers over time and its implication for
    the search for life on extrasolar Earth-like planets. We show that
    atmospheric features on Earth can provide clues of biological activities for
    at least 2 billion years.

    \\ ( http://arXiv.org/abs/astro-ph/0512053 , 391kb)


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