Exoplanet astronomy; Stellar activity; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] We present mass and radius measurements of K2-79b and K2-222b, two transiting exoplanets orbiting active G-type stars observed with HARPS-N and K2. Their respective 10.99 day and 15.39 day orbital periods fall near periods of signals induced by stellar magnetic activity. The two signals might therefore interfere and lead to an inaccurate estimate of exoplanet mass. We present a method to mitigate these effects when radial velocity (RV) and activity-indicator observations are available over multiple observing seasons and the orbital period of the exoplanet is known. We perform correlation and periodogram analyses on subsets composed of each target's two observing seasons, in addition to the full data sets. For both targets, these analyses reveal an optimal season with little to no interference at the orbital period of the known exoplanet. We make a confident mass detection of each exoplanet by confirming agreement between fits to the full RV set and the optimal season. For K2-79b, we measure a mass of 11.8 ± 3.6 M ⊕ and a radius of 4.09 ± 0.17 R ⊕. For K2-222b, we measure a mass of 8.0 ± 1.8 M ⊕ and a radius of 2.35 ± 0.08 R ⊕. According to model predictions, K2-79b is a highly irradiated Uranus analog and K2-222b hosts significant amounts of water ice. We also present a RV solution for a candidate second companion orbiting K2-222 at 147.5 days.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Nava, Chantanelle ; Center for Astrophysics | Harvard and Smithsonian, Cambridge, United States
López-Morales, Mercedes ; Center for Astrophysics | Harvard and Smithsonian, Cambridge, United States
Mortier, Annelies ; Astrophysics Group, Cavendish Laboratory, University of Cambridge, Cambridge, United Kingdom ; Kavli Institute for Cosmology, University of Cambridge, Cambridge, United Kingdom
Zeng, Li ; Center for Astrophysics | Harvard and Smithsonian, Cambridge, United States ; Department of Earth and Planetary Sciences, Harvard University, Cambridge, United States
Giles, Helen A. C. ; Observatoire de Geneve, Université de Geneve, Sauverny, Switzerland
Bieryla, Allyson ; Center for Astrophysics | Harvard and Smithsonian, Cambridge, United States
Vanderburg, Andrew ; Department of Astronomy, University of Wisconsin, Madison, United States
Buchhave, Lars A. ; DTU Space, National Space Institute, Technical University of Denmark, Lyngby, Denmark
Sasselov, Dimitar ; Center for Astrophysics | Harvard and Smithsonian, Cambridge, United States
Mayor, Michel ; Observatoire de Geneve, Université de Geneve, Sauverny, Switzerland
Stalport, Manu ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR) ; Observatoire de Geneve, Université de Geneve, Sauverny, Switzerland
Malavolta, Luca ; INAFOsservatorio Astronomico di Padova, Padova, Italy ; Dipartimento di Fisica e Astronomia "galileo Galilei, Universitá di Padova, Padova, Italy
Rice, Ken; SUPA, Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, United Kingdom ; Centre for Exoplanet Science, University of Edinburgh, Edinburgh, United Kingdom
Watson, Christopher A.; Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast, United Kingdom