Jim Davenport from the University of Washington will review some of the transformative discoveries enabled by Kepler and TESS.

Core-collapse supernova explosions (CCSN) are one possible fate of a massive star. Simulations of CCSNe rely on the properties of the massive star at core-collapse.

David Weinberg from Ohio State University will present on “Decoding Chemical Evolution and Nucleosynthesis”

A presentation on the High-efficiency Instrument for the Rapid Assessment of eXo-atmospheres (HIRAX) by Ashley Baker