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Response of Atmospheric Biomarkers to NO(x)-Induced Photochemistry Generated by Stellar Cosmic Rays for Earth-like Planets in the Habitable Zone of M Dwarf Stars
Understanding whether M dwarf stars may host habitable planets with Earth-like atmospheres and biospheres is a major goal in exoplanet research. If such planets exist, the question remains as to whether they could be identified via spectral signatures of biomarkers. Such planets may be exposed to ex...
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| Main Authors: | , , , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Mary Ann Liebert, Inc.
2012
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3522229/ https://ncbi.nlm.nih.gov/pubmed/23215581 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2011.0682 |
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