A black hole is a region of spacetime where gravity is so strong that nothing, not even light, can escape. Most form when the core of a massive star collapses at the end of its life, compressing matter past a critical density. Every black hole is described by just three properties: mass, spin, and electric charge. Its boundary is the event horizon, and at its center general relativity predicts a singularity where the theory itself breaks down. The Event Horizon Telescope has now imaged the glowing ring of light around two of them, in the galaxy M87 and at the center of the Milky Way.
Cosmology · Early Universe · Black Holes
When JWST looked deep into the early universe, it found a swarm of tiny, intensely red points of light. The leading answer would mean black holes appe...
Cosmology · Dark Matter · Black Holes
Stars cannot leave a black hole lighter than the Sun. In late 2025 a gravitational-wave detector caught a signal hinting at exactly that, possibly a r...
Cosmology · Gravitational Waves · Black Holes
Theory assumed colliding compact objects settle into near-perfect circles before merging. Then astronomers reanalyzed a black hole swallowing a neutro...
Astrophysics · Black Holes · Tidal Disruption
Wander too close to a supermassive black hole and gravity becomes a weapon. The star is stretched into a stream of gas, half of it swallowed in a flar...
Cosmology · Gravitational Waves · Black Holes
In one release, the number of gravitational-wave detections more than doubled. The fourth LIGO-Virgo-KAGRA catalog turned a handful of collisions into...
Astrophysics · Supernovae · Black Holes
A star 730 million light-years away brightened for four years, exploded, then exploded again. No human flagged it. An algorithm built to find the stra...