Habitable moons around extrasolar giant planets

@article{Williams1997HabitableMA,
  title={Habitable moons around extrasolar giant planets},
  author={Darren M. Williams and James F Kasting and Richard Alan Wade},
  journal={Nature},
  year={1997},
  volume={385},
  pages={234-236}
}
Possible planetary objects have now been discovered1–9 orbiting nine different main-sequence stars. These companion objects (some of which might actually be brown dwarfs) all have a mass at least half that of Jupiter, and are therefore unlikely to be hospitable to Earth-like life: jovian planets and brown dwarfs support neither a solid nor a liquid surface near which organisms might dwell. Here we argue that rocky moons orbiting these companions could be habitable if the planet–moon system… 
Transits of extrasolar moons around luminous giant planets
Beyond Earth-like planets, moons can be habitable, too. No exomoons have been securely detected, but they could be extremely abundant. Young Jovian planets can be as hot as late M stars, with
Looking for planetary moons in the spectra of distant Jupiters.
TLDR
A possible way of detecting Earth-sized moons with future technology by taking advantage of spectral contrast of Jovian-sized planets near the habitable zones of main-sequence stars to discern which extrasolar giant planets have Earth-like moons capable of supporting life.
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Resonant Removal of Exomoons During Planetary Migration
Jupiter and Saturn play host to an impressive array of satellites, making it reasonable to suspect that similar systems of moons might exist around giant extrasolar planets. Furthermore, a
MAGNETIC SHIELDING OF EXOMOONS BEYOND THE CIRCUMPLANETARY HABITABLE EDGE
With most planets and planetary candidates detected in the stellar habitable zone (HZ) being super-Earths and gas giants rather than Earth-like planets, we naturally wonder if their moons could be
Stability of Satellites around Close-in Extrasolar Giant Planets
We investigate the long-term dynamical stability of hypothetical moons orbiting extrasolar giant planets. Stellar tides brake a planet's rotation and, together with tidal migration, act to remove
THE POTENTIAL FOR TIDALLY HEATED ICY AND TEMPERATE MOONS AROUND EXOPLANETS
Moons of giant planets may represent an alternative to the classical picture of habitable worlds. They may exist within the circumstellar habitable zone of a parent star, and through tidal energy
Worlds without Moons: Exomoon Constraints for Compact Planetary Systems
One of the primary surprises of exoplanet detections has been the discovery of compact planetary systems, whereby numerous planets reside within ~0.5 au of the host star. Many of these kinds of
Tides, planetary companions, and habitability: habitability in the habitable zone of low-mass stars
Earth-scale planets in the classical habitable zone (HZ) are more likely to be habitable if they possess active geophysics. Without a constant internal energy source, planets cool as they age,
Habitable planets around white and brown dwarfs: the perils of a cooling primary.
TLDR
The future habitability of the planet candidates KOI 55.01 and 55.02 is considered in these terms and it is found they are unlikely to become habitable.
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