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