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The launch of NASA's Kepler space telescope in 2009 revolutionized thequality and quantity of observational data available for asteroseismicanalysis. While Kepler was able to detect solar-like oscillations in hundredsof main-sequence and subgiant stars, the Transiting Exoplanet Survey Satellite(TESS) is now making similar observations for thousands of the brightest starsin the sky. The Asteroseismic Modeling Portal (AMP) is an automated andobjective stellar model-fitting pipeline for asteroseismic data, which wasoriginally developed to use models from the Aarhus Stellar Evolution Code(ASTEC). We briefly summarize an updated version of the AMP pipeline that usesModules for Experiments in Stellar Astrophysics (MESA), and we present initialmodeling results for the Sun and several solar analogs to validate theprecision and accuracy of the inferred stellar properties.

Overview and Validation of the Asteroseismic Modeling Portal v2.0