A bright ring of light around a black hole formed by photons orbiting near the event horizon.The photon ring is the bright, thin halo of light that appears around a black hole's shadow when we observe it. It is not light emitted by the black hole itself — nothing escapes from inside the event horizon — but rather light from distant stars or hot gas that gets bent by the black hole's extreme gravity. Some of that light loops around the black hole one or more times before reaching our telescopes, creating a distinctive ring that is a direct visual signature of the warped spacetime.
The concept of a photon sphere was first derived by David Finkelstein and others in the late 1950s, and the term 'photon ring' became prominent with the 2019 Event Horizon Telescope image of M87*. The detailed theory of photon rings as observable features was developed by astronomers like Avery Broderick and Avi Loeb in the 2000s.
Photons passing near a black hole follow curved paths dictated by general relativity. Those that come within a certain critical distance — the photon sphere, at 1.5 times the Schwarzschild radius for a non-rotating black hole — can be deflected so strongly that they orbit the black hole several times. The light that escapes after these loops arrives at our detectors slightly delayed and concentrated into a narrow ring. The ring's size and shape encode the black hole's mass and spin, while its brightness distribution can reveal chaotic photon trajectories and even subtle effects from dark matter or modified gravity.
Photon rings are used to measure black hole spin and test general relativity in strong gravity, and they are a key target for next-generation very-long-baseline interferometry (VLBI) arrays like the Event Horizon Telescope.
The photon ring of a black hole can be up to several times brighter than the surrounding accretion disk because light can loop around the black hole multiple times, effectively amplifying the signal.










