Habitable Zones Around Main-Sequence Stars: New Estimates

@article{Kopparapu2013HabitableZA,
  title={Habitable Zones Around Main-Sequence Stars: New Estimates},
  author={R. Kopparapu and R. Ramirez and J. Kasting and V. Eymet and T. Robinson and S. Mahadevan and R. Terrien and S. Domagal-Goldman and V. Meadows and R. Deshpande},
  journal={The Astrophysical Journal},
  year={2013},
  volume={765},
  pages={131}
}
Identifying terrestrial planets in the habitable zones (HZs) of other stars is one of the primary goals of ongoing radial velocity (RV) and transit exoplanet surveys and proposed future space missions. Most current estimates of the boundaries of the HZ are based on one-dimensional (1D), cloud-free, climate model calculations by Kasting et?al. However, this model used band models that were based on older HITRAN and HITEMP line-by-line databases. The inner edge of the HZ in the Kasting et?al… Expand

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