# The Hunt for Exomoons with Kepler (HEK). III. The First Search for an Exomoon around a Habitable-zone Planet

## Author(s): Kipping, DM; Forgan, D; Hartman, J; Nesvorný, D; Bakos, Gaspar Aron; et al

To refer to this page use: http://arks.princeton.edu/ark:/88435/pr13m62
DC FieldValueLanguage
dc.contributor.authorKipping, DM-
dc.contributor.authorForgan, D-
dc.contributor.authorHartman, J-
dc.contributor.authorNesvorný, D-
dc.contributor.authorBakos, Gaspar Aron-
dc.contributor.authorSchmitt, A-
dc.contributor.authorBuchhave, L-
dc.date.accessioned2019-04-10T19:31:09Z-
dc.date.available2019-04-10T19:31:09Z-
dc.date.issued2013-11-10en_US
dc.identifier.citationKipping, DM, Forgan, D, Hartman, J, Nesvorný, D, Bakos, GÁ, Schmitt, A, Buchhave, L. (2013). The Hunt for Exomoons with Kepler (HEK). III. The First Search for an Exomoon around a Habitable-zone Planet. \apj, 777 (134 - 134. doi:10.1088/0004-637X/777/2/134en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr13m62-
dc.description.abstractKepler-22b is the first transiting planet to have been detected in the habitable zone of its host star. At 2.4 R ⊕ , Kepler-22b is too large to be considered an Earth analog, but should the planet host a moon large enough to maintain an atmosphere, then the Kepler-22 system may yet possess a telluric world. Aside from being within the habitable zone, the target is attractive due to the availability of previously measured precise radial velocities and low intrinsic photometric noise, which has also enabled asteroseismology studies of the star. For these reasons, Kepler-22b was selected as a target-of-opportunity by the “Hunt for Exomoons with Kepler” (HEK) project. In this work, we conduct a photodynamical search for an exomoon around Kepler-22b leveraging the transits, radial velocities, and asteroseismology plus several new tools developed by the HEK project to improve exomoon searches. We find no evidence for an exomoon around the planet and exclude moons of mass M S > 0 . 5 M ⊕ to 95% confidence. By signal injection and blind retrieval, we demonstrate that an Earth-like moon is easily detected for this planet even when the time-correlated noise of the data set is taken into account. We provide updated parameters for the planet Kepler-22b, including a revised mass of M P < 53 M ⊕ to 95% confidence and an eccentricity of 0 . 13 +0 . 36 − 0 . 13 by exploiting Single-body Asterodensity Profiling. Finally, we show that Kepler-22b has a > 95% probability of being within the empirical habitable zone but a < 5% probability of being within the conservative habitable zone.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstrophysical Journalen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleThe Hunt for Exomoons with Kepler (HEK). III. The First Search for an Exomoon around a Habitable-zone Planeten_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-637X/777/2/134-
dc.date.eissued2013-10-22en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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