The evolution of habitable zones during stellar lifetimes and its implications on the search for extraterrestrial life

@article{Underwood2003TheEO,
  title={The evolution of habitable zones during stellar lifetimes and its implications on the search for extraterrestrial life},
  author={D. R. Underwood and B. Jones and P. N. Sleep},
  journal={International Journal of Astrobiology},
  year={2003},
  volume={2},
  pages={289 - 299}
}
A stellar evolution computer model has been used to determine changes in the luminosity L and effective temperature Te of single stars during their time on the main sequence. The range of stellar masses investigated was from 0.5 to 1.5 times that of the Sun, each with a mass fraction of metals (metallicity, Z) from 0.008 to 0.05. The extent of each star's habitable zone (HZ) has been determined from its values of L and Te. These stars form a reference framework for other main sequence stars… Expand
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