From galaxy rotations to gravitational lensing, dark matter leaves its fingerprints in gravity alone. In this episode, we zoom in on ultra-faint dwarf galaxies orbiting the Milky Way—tiny, dark-matter–dominated laboratories that help us pin down dark matter’s mass. We’ll explore the idea that ultra-light, wave-like dark matter could create fuzzy cores, and how precise stellar motions in Leo II are used to set bounds on the particle mass—without heavy assumptions. Join us for a data-driven journey through one of the universe’s most intriguing mysteries and how these diminutive galaxies are reshaping our understanding of the dark sector.
Note: This podcast was AI-generated, and sometimes AI can make mistakes. Please double-check any critical information.
Sponsored by Embersilk LLC