Biosignatures and extrasolar planet characterization: visible versus infrared

Details Biosignatures and extrasolar planet characterization: visible versus infrared Biosignatures and extrasolar planet characterization: visible versus infrared

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.539..205s&link_type=abstract

In: Proceedings of the Conference on Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets, 22-25 A

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Biosignature, Planet Characterization, Visible, Infrared

Scientific paper

The physical bases of the detection and characterisation of extrasolar Earth-like planets and of biosignatures in the reflected light and thermal emission regimes are reviewed. Both approaches have their advantages and disadvantages, including artefacts, in the determination of planet physical parameters (mass, size, albedo, surface and atmospheric conditions etc.) and biosignatures. New perspectives for these different aspects are presented.

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