![]() ![]() Significant outcomes of our modeling efforts include a precise prediction for the star's radius. Our theoretical predictions include self-consistent results from multi-timescale evolutionary, oscillatory, and hydrodynamic simulations conducted with the Modules for Experiments in Stellar Astrophysics software suite. We detect the first radial overtone in the photometric data and report a period of 185 ± 13.5 days. Our observational results include the release of new, processed photometric measurements collected with the space-based Solar Mass Ejection Imager instrument prior to Betelgeuse's recent, unprecedented dimming event. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan conduct a rigorous examination of the nearby red supergiant Betelgeuse by drawing on the synthesis of new observational data and three different modeling techniques. MTA CSFK Lendulet Near-Field Cosmology Research Group, Konkoly-Thege út 15-17, H-1121 Budapest, HungaryĮLTE Eotvs Loránd University, Institute of Physics, Budapest, 1117, Pázmány Péter sétány 1/A, HungaryĬentre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, Caltech, Pasadena, CA 91125, USA Observatory, Research Centre for Astronomy and Earth Sciences, Konkoly-Thege út 15-17, H-1121 Budapest, Hungary ![]() ![]() ![]() Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia ![]()
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