This book shows how transiting planets may be used to infer the presence of exomoons through deviations in time and duration of planetary eclipses. It shows that habitable-zone exomoons above 0.2 Earth-masses can be detected with the Kepler space telescope.

This book shows how transiting planets may be used to infer the presence of exomoons through deviations in time and duration of planetary eclipses. It shows that habitable-zone exomoons above 0.2 Earth-masses can be detected with the Kepler space telescope.

This book shows how transiting planets may be used to infer the presence of exomoons through deviations in time and duration of planetary eclipses. It shows that habitable-zone exomoons above 0.2 Earth-masses can be detected with the Kepler space telescope.