Supermassive black holes

Nearly every large galaxy harbors a supermassive black hole at its center, with masses millions to billions of times that of the Sun. But these objects are notoriously hard to study directly. JWST has transformed the field, finding dormant black holes at cosmological distances by watching stars orbit an invisible center, and piercing the dusty cocoons around active black holes in the early universe. Closer to home, the Milky Way's own central black hole, Sagittarius A*, is a natural laboratory for understanding how these cosmic giants interact with their surroundings.


Black hole mergers

When two black holes collide, they send ripples through the fabric of spacetime itself. LIGO, Virgo, and KAGRA have now detected nearly 400 such events, charting the population of black holes across the universe. The latest catalog includes the best-localized gravitational wave source ever found, the clearest signal ever recorded, and hints of black holes that are themselves the products of earlier mergers. Each event is a snapshot of a universe where gravity is at its most extreme.


Mysteries and alternatives

For all that we have learned about black holes, deep questions remain. Theoretical physicists have found a solution to Einstein's equations in which a collapsing star does not form a black hole at all, but instead creates a tiny expanding universe inside, a gravastar. Meanwhile, a dust-shrouded galaxy 11 billion light-years away confounded expectations by producing neutrinos without a black hole at its core, powered instead by star formation alone. These stories remind us that the universe is stranger than our models predict, and that the next discovery may upend what we think we know.