Climatological and UV-based Habitability of Possible Exomoons in F-star Systems

@article{Sato2015ClimatologicalAU,
  title={Climatological and UV-based Habitability of Possible Exomoons in F-star Systems},
  author={S. Sato and Zh. Wang and Manfred Cuntz},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2015}
}
We explore the astrobiological significance of F-type stars of spectral type between F5 V and F9.5 V, which possess Jupiter-type planets within or close to their climatological habitable zones. These planets, or at least a subset of those, may also possess rocky exomoons, which potentially offer habitable environments. Our work considers eight selected systems. The Jupiter-type planets in these systems are in notably differing orbits with eccentricities between 0.08 (about Mars) and 0.72. We… 

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