Transmission spectra of terrestrial exoplanets in the IR

Details Transmission spectra of terrestrial exoplanets in the IR Transmission spectra of terrestrial exoplanets in the IR

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007epsc.conf..802c&link_type=abstract

European Planetary Science Congress 2007, Proceedings of a conference held 20-24 August, 2007 in Potsdam, Germany. Online at ht

Physics

Scientific paper

The next generation of space telescopes (James Webb Space Telescope, JWST, 2013) will have the capability of acquiring spectra of smaller extrasolar worlds. To understand our ability to characterize neptune- and earth-size transiting exoplanets, we have generated synthetic transmission spectra of these exotic environments, using a set of chemistry, climate and radiative transfer models. In this presentation we will focus on the detectability of spectral signatures of crucial atmospheric molecules with future observations.

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