Habitability of Known Exoplanetary Systems Based on Measured Stellar Properties

@article{Jones2006HabitabilityOK,
  title={Habitability of Known Exoplanetary Systems Based on Measured Stellar Properties},
  author={B. Jones and P. N. Sleep and D. R. Underwood},
  journal={The Astrophysical Journal},
  year={2006},
  volume={649},
  pages={1010-1019}
}
Habitable planets are likely to be broadly Earth-like in composition, mass, and size. Masses are likely to be within a factor of a few of the Earth's mass. Currently, we do not have sufficiently sensitive techniques to detect Earth-mass planets, except in rare circumstances. It is thus necessary to model the known exoplanetary systems. In particular, we need to establish whether Earth-mass planets could be present in the classical habitable zone (HZ) or whether the giant planets that we know to… Expand
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