1. WASP-131 b with ESPRESSO – I. A bloated sub-Saturn on a polar orbit around a differentially rotating solar-type star.
- Author
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Doyle, L, Cegla, H M, Anderson, D R, Lendl, M, Bourrier, V, Bryant, E, Vines, J, Allart, R, Bayliss, D, Burleigh, M R, Buchschacher, N, Casewell, S L, Hawthorn, F, Jenkins, J S, Lafarga, M, Moyano, M, Psaridi, A, Roguet-Kern, N, Sosnowska, D, and Wheatley, P
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ORBITS (Astronomy) , *STELLAR rotation , *ESPRESSO , *LIGHT curves , *PLANETARY systems , *SATURN (Planet) - Abstract
In this paper, we present observations of two high-resolution transit data sets obtained with ESPRESSO of the bloated sub-Saturn planet WASP-131 b. We have simultaneous photometric observations with NGTS and EulerCam. In addition, we utilized photometric light curves from TESS , WASP, EulerCam, and TRAPPIST of multiple transits to fit for the planetary parameters and update the ephemeris. We spatially resolve the stellar surface of WASP-131 utilizing the Reloaded Rossiter McLaughlin technique to search for centre-to-limb convective variations, stellar differential rotation, and to determine the star–planet obliquity for the first time. We find WASP-131 is misaligned on a nearly retrograde orbit with a projected obliquity of |$\lambda = 162.4\substack{+1.3 \\ -1.2}^{\circ }$|. In addition, we determined a stellar differential rotation shear of α = 0.61 ± 0.06 and disentangled the stellar inclination (|$i_* = 40.9\substack{+13.3 \\ -8.5}^{\circ }$|) from the projected rotational velocity, resulting in an equatorial velocity of |$v_{\rm {eq}} = 7.7\substack{+1.5 \\ -1.3}$| km s−1. In turn, we determined the true 3D obliquity of |$\psi = 123.7\substack{+12.8 \\ -8.0}^{\circ }$| , meaning the planet is on a perpendicular/polar orbit. Therefore, we explored possible mechanisms for the planetary system's formation and evolution. Finally, we searched for centre-to-limb convective variations where there was a null detection, indicating that centre-to-limb convective variations are not prominent in this star or are hidden within red noise. [ABSTRACT FROM AUTHOR]
- Published
- 2023
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