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Redshifted Sodium Transient near Exoplanet Transit
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Redshifted Sodium Transient near Exoplanet Transit
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Redshifted Sodium Transient near Exoplanet Transit
Redshifted Sodium Transient near Exoplanet Transit
Paper

Redshifted Sodium Transient near Exoplanet Transit

2024
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Overview
Neutral sodium (Na I) is an alkali metal with a favorable absorption cross section such that tenuous gases are easily illuminated at select transiting exoplanet systems. We examine both the time-averaged and time-series alkali spectral flux individually, over 4 nights at a hot Saturn system on a \\(\\) 2.8 day orbit about a Sun-like star WASP-49 A. Very Large Telescope/ESPRESSO observations are analyzed, providing new constraints. We recover the previously confirmed residual sodium flux uniquely when averaged, whereas night-to-night Na I varies by more than an order of magnitude. On HARPS/3.6-m Epoch II, we report a Doppler redshift at \\(v_ NaD =\\) +9.7 \\(\\) 1.6 km/s with respect to the planet's rest frame. Upon examining the lightcurves, we confirm night-to-night variability, on the order of \\(\\) 1-4 % in NaD rarely coinciding with exoplanet transit, not readily explained by stellar activity, starspots, tellurics, or the interstellar medium. Coincident with the \\(\\)+10 km/s Doppler redshift, we detect a transient sodium absorption event dF\\(_NaD\\)/F\\(_\\) = 3.6 \\(\\) 1 % at a relative difference of \\( F_NaD (t) \\) 4.4 \\(\\) 1 %, enduring \\( t_NaD \\) 40 minutes. Since exoplanetary alkali signatures are blueshifted due to the natural vector of radiation pressure, estimated here at roughly \\(\\) -5.7 km/s, the radial velocity is rather at +15.4 km/s, far larger than any known exoplanet system. Given that the redshift magnitude v\\(_\\) is in between the Roche limit and dynamically stable satellite orbits, the transient sodium may be a putative indication of a natural satellite orbiting WASP-49 A b.