The impact of two non-transiting planets and stellar activity on mass determinations for the super-Earth CoRoT-7b
Date
01/09/2022Funder
Grant ID
ST/R00824/1
ST/R003203/1
ST/V000861/1
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Show full item recordAbstract
CoRoT-7 is an active star, whose orbiting planets and their masses have been under debate since their initial detection. In the previous studies, CoRoT-7 was found to have two planets, CoRoT-7b and CoRoT-7c with orbital periods 0.85 and 3.69 d, and a potential third planet with a period ∼9 d. The existence of the third planet has been questioned later as potentially being an activity-induced artefact. Moreover, mass of the transiting planet CoRoT-7b has been estimated to have widely different values owing to the activity level of the parent star, the consequent RV ‘jitter’, and the methods used to rectify this ambiguity. Here, we present an analysis of the HARPS archival RV (RV) data of CoRoT-7 using a new wavelength-domain technique, SCALPELS, to correct for the stellar activity-induced spectral line-shape changes. Simultaneous modelling of stellar activity and orbital motions, identified using the l1- periodogram, shows that SCALPELS effectively reduce the contribution of stellar variability to the RV signal and enhance the detectability of exoplanets around active stars. Using KIMA nested-sampling package (Faria et al.), we modelled the system incorporating a Gaussian Process together with SCALPELS. The resultant posterior distributions favoured a three-planet system comprising two non-transiting planets, CoRoT-7c and CoRoT-7d with orbital periods 3.697 ± 0.005 and 8.966 ± 1.546 d, in addition to the known transiting planet. The transiting planet CoRoT-7b is found to be a rocky super-Earth with a mass of Mb = 6.06 ± 0.65M⊕. The determined masses of Mc = 13.29 ± 0.69M⊕ and Md = 17.14 ± 2.55M⊕ suggest the non-transiting planets CoRoT-7c and CoRoT-7d to be structurally similar to Uranus and Neptune.
Citation
Anna John , A , Cameron , A C & Wilson , T G 2022 , ' The impact of two non-transiting planets and stellar activity on mass determinations for the super-Earth CoRoT-7b ' , Monthly Notices of the Royal Astronomical Society , vol. 515 , no. 3 , pp. 3975-3995 . https://doi.org/10.1093/mnras/stac1814
Publication
Monthly Notices of the Royal Astronomical Society
Status
Peer reviewed
ISSN
0035-8711Type
Journal article
Description
Funding: AAJ acknowledges the support from World leading St Andrews Doctoral Scholarship. ACC and TGW acknowledge support from STFC consolidated grant numbers ST/R000824/1 and ST/V000861/1, and UKSA grant number ST/R003203/1.Collections
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