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Detectability of planetary characteristics from spatially and spectrally-resolved models of terrestrial planets: Mars and Earth

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dc.contributor.author Tinetti, G. en_US
dc.contributor.author Crisp, D. en_US
dc.contributor.author Meadows, V. S. en_US
dc.contributor.author Velusamy, T. en_US
dc.contributor.author Kasting, J. F. en_US
dc.contributor.author Segura, A. en_US
dc.contributor.author Krelove, K. en_US
dc.contributor.author Fong, W. en_US
dc.contributor.author Snively, H. en_US
dc.date.accessioned 2004-09-16T23:54:10Z
dc.date.available 2004-09-16T23:54:10Z
dc.date.issued 2003-09-02 en_US
dc.identifier.citation American Astronomical Society's Division of Planetary Science 2003 Annual Meeting en_US
dc.identifier.citation Monterey, CA, USA en_US
dc.identifier.clearanceno 03-2599 en_US
dc.identifier.uri http://hdl.handle.net/2014/7917
dc.description.abstract The principal goal of the NASA Terrestrial Planet Finder mission is to detect and characterize extrasolar terrestrial planets. en_US
dc.format.extent 3262211 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other astrobiology extrasolar planets remote sensing en_US
dc.title Detectability of planetary characteristics from spatially and spectrally-resolved models of terrestrial planets: Mars and Earth en_US


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