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Thermodynamic Limits Around M-dwarf Stars: Orbital Distances and Incident Spectral Fluxesby@photosynthesis
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Thermodynamic Limits Around M-dwarf Stars: Orbital Distances and Incident Spectral Fluxes

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In this study, researchers explore the feasibility and potential characteristics of photosynthetic light-harvesting on exo-planets.
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(1) Samir Chitnavis, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK & Digital Environment Research Institute, Queen Mary University of London, Empire House, Whitechapel E1 1HH, UK;

(2) Thomas J. Haworth, Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK;

(3) Edward Gillen, Astronomy Unit, Queen Mary University of London, Mile End Road, London E1 4NS, UK;

(4) Conrad W. Mullineaux, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK;

(5) Christopher D. P. Duffy, School of Biological and Behavioural Sciences, Queen Mary University of London, Mile End, London E1 4NS, UK & Digital Environment Research Institute, Queen Mary University of London, Empire House, Whitechapel E1 1HH, UK (Email: [email protected]).

3 Results

3.1 Orbital distances and incident spectral fluxes





This paper is available on arxiv under CC 4.0 license.