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  5. K2-79b and K2-222b: Mass Measurements of Two Small Exoplanets with Periods beyond 10 days that Overlap with Periodic Magnetic Activity Signals
 

K2-79b and K2-222b: Mass Measurements of Two Small Exoplanets with Periods beyond 10 days that Overlap with Periodic Magnetic Activity Signals

Journal
THE ASTRONOMICAL JOURNAL  
Date Issued
2022
Author(s)
Nava, Chantanelle
•
López-Morales, Mercedes
•
Mortier, Annelies
•
Zeng, Li
•
Giles, Helen A.C.
•
Bieryla, Allyson
•
Vanderburg, Andrew
•
Buchhave, Lars A.
•
PORETTI, Ennio  
•
Saar, Steven H.
•
Dumusque, Xavier
•
Latham, David W.
•
Charbonneau, David
•
Damasso, Mario  
•
BONOMO, ALDO STEFANO  
•
Lovis, Christophe
•
Collier Cameron, Andrew
•
Eastman, Jason D.
•
SOZZETTI, Alessandro  
•
COSENTINO, Rosario  
•
Pedani, Marco
•
Pepe, Francesco
•
MOLINARI, Emilio Carlo  
•
Sasselov, Dimitar
•
Mayor, Michel
•
Stalport, Manu
•
Malavolta, Luca
•
Rice, Ken
•
Watson, Christopher A.
•
Martinez Fiorenzano, A. F.
•
DI FABRIZIO, LUCA  
DOI
10.3847/1538-3881/ac3141
Abstract
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.
Volume
163
Issue
2
Start page
41
Uri
http://hdl.handle.net/20.500.12386/32033
Url
https://api.elsevier.com/content/abstract/scopus_id/85122720705
https://iopscience.iop.org/article/10.3847/1538-3881/ac3141
Issn Identifier
0004-6256
Rights
open.access
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