The Effects of Stellar Gravity Darkening on High-resolution Transmission Spectra

Abstract

Abstract High-resolution transmission spectroscopy is a powerful method for probing the extended atmospheres of short-period exoplanets. With the advancement of ultrastable echelle spectrographs and the advent of 30 m class telescopes on the horizon, even minor observational and physical effects will become important when modeling atmospheric absorption of atomic species. In this work we demonstrate how the nonuniform temperature across the surface of a fast rotating star, i.e., gravity darkening, can affect the observed transmission spectrum in a handful of atomic transitions commonly observed in short-period exoplanet atmospheres. We simulate transits of the ultrahot Jupiters KELT-9 b and HAT-P-70 b but our results are applicable to all short-period gas giants transiting rapidly rotating stars. In general, we find that gravity darkening has a small effect on the average transmission spectrum but can change the shape of the absorption light curve, similar to the effect observed in broadband photometric transits. While the magnitude of gravity-darkening effects are on the same order as the noise in transmission spectra observed with 10 m class telescopes, future high-quality spectroscopic light curves for individual atomic absorption lines collected with 30 m class telescopes will need to account for this effect.