When a star at its life's end explodes, a debris cloud expands away from the now-dead star. The debris forms intricate and amazing structures in the expanding cloud and can cause the formation of a variety of molecules. Using the James Webb Space Telescope, scientists have collected information regarding Cassiopeia A (Cas A), the youngest known supernova remnant in the Milky Way. The observations shed light on how molecules and dust form and are destroyed in the aftermath of an explosion. These results suggest that supernovae, like Cas A, are key sources of the dust observed in ancient galaxies. A recent paper highlights the findings of this work, including the temperatures measured and molecules formed. Deputy Director of the Carl Sagan Center Simon Steel chats with lead author Jeonghee Rho and co-authors Danny Milisavljevic and Ilse De Looze about the data collected and what it means for dust formation in the universe. (Recorded live 29 August 2024.)