The Age Dependence of the Detectability of Comets Orbiting Solar-Type Stars

@article{Jura2005TheAD,
  title={The Age Dependence of the Detectability of Comets Orbiting Solar-Type Stars},
  author={M. Jura},
  journal={The Astrophysical Journal},
  year={2005},
  volume={620},
  pages={487 - 491}
}
  • M. Jura
  • Published 28 October 2004
  • Physics, Geology
  • The Astrophysical Journal
The outflows from comets in orbit around G-type main-sequence stars can be detected when they produce transient OH absorption lines in the spectrum near 3100 Å of the host star. There is only about a 3 × 10-8 probability of detecting an analog to comet Hale-Bopp orbiting an analog to the Sun. However, for young solar-type stars with very large numbers of comets, possibly delivering water to terrestrial planets, there is as much as a 1% chance that any sufficiently sensitive, randomly timed… 

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