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The detectability of habitable exomoons

Published online by Cambridge University Press:  21 October 2010

David M. Kipping
Affiliation:
University College London, Dept. of Physics & Astronomy, Gower Stree, London, N1 0XE, UK email: d.kipping@ucl.ac.uk
Stephen J. Fossey
Affiliation:
University College London, Dept. of Physics & Astronomy, Gower Stree, London, N1 0XE, UK email: d.kipping@ucl.ac.uk
Giammarco Campanella
Affiliation:
University College London, Dept. of Physics & Astronomy, Gower Stree, London, N1 0XE, UK email: d.kipping@ucl.ac.uk
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Abstract

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Despite the number of known exoplanets increasing on an almost weekly basis, the question as to whether exoplanets host moons remains unanswered. Exomoons could be potential seats for life, as well as improving our understanding of planetary formation and celestial mechanics. Here we summarize our findings from an investigation into how detectable habitable-zone exomoons are with Kepler-class photometry.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

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