BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Variable atmospheric dynamics of planets experiencing gravity-dark ened seasons DTSTART;VALUE=DATE-TIME:20220907T103000Z DTEND;VALUE=DATE-TIME:20220907T104500Z DTSTAMP;VALUE=DATE-TIME:20240704T115908Z UID:indico-contribution-124@meetings.aip.de DESCRIPTION:Speakers: Anusha Pai Asnodkar (The Ohio State University)\nPla nets on misaligned orbits around rapid rotators can experience “gravity- darkened seasons” as their orbits cross over the hot poles and cooler eq uators of rotationally-flattened stars. The periodically variable heating from these seasons presents a unique case for exploring how changes in ste llar irradiation influence planetary atmospheric dynamics. We perform a ho mogeneous analysis of day-to-nightside winds on the ultra-hot Jupiters KEL T-9 b and KELT-20 b\, enabling the comparison of a planet experiencing gra vity-darkened seasons (KELT-9 b) with a similar planet that does not (KELT -20 b). We conduct high-resolution transmission spectroscopy using two tra nsits observed by the PEPSI spectrograph on the Large Binocular Telescope to empirically constrain supersonic ~10 km/s day-to-nightside winds traced by Fe II features in the atmosphere of KELT-9 b. Reconciling our findings with two archival HARPS-N datasets suggests multi-epoch variability ~5-8 km/s over timescales between weeks to years. In contrast\, KELT-20 b’s d ay-to-nightside winds are less rapid (~2 km/s) and stable across four tran sits collectively observed by PEPSI and HARPS-N. The observed contrast of KELT-9 b’s wind variability and KELT-20 b’s stability is in accordance with our intuition on the effect of gravity-darkened seasons. A qualitati ve evaluation of our measured wind velocities and variability against curr ent ultra-hot Jupiter GCMs reveals that KELT-9 b poses unique challenges f or validating giant planet atmospheric models.\n\nhttps://meetings.aip.de/ event/16/contributions/124/ LOCATION:Leibniz Institute for Astrophysics Potsdam (AIP) Lecture Hall URL:https://meetings.aip.de/event/16/contributions/124/ END:VEVENT END:VCALENDAR