The narrowest part of a wormhole through which light passes.In the context of wormholes, the throat is the narrowest cross-section of the tunnel connecting two distant regions of spacetime. It is the point where the gravitational potential is highest and where the geometry of the wormhole is most constrained. Light and matter passing through a wormhole must traverse this bottleneck, and its properties — size, shape, and rotation — determine what can pass through and how it appears to outside observers.
The concept of a wormhole throat was formalized in the 1930s by Albert Einstein and Nathan Rosen, who proposed a bridge connecting two identical regions of spacetime — now called the Einstein–Rosen bridge. The modern notion of a traversable throat with exotic matter was developed by Kip Thorne and Michael Morris in 1988.
The throat is defined by the minimal radius of the wormhole's spatial cross-section. In a traversable wormhole, the throat must be held open against gravitational collapse, which typically requires exotic matter with negative energy density. The throat's geometry affects light rays: they are deflected, focused, or even trapped near it, creating characteristic shadows and lensing patterns. If the wormhole rotates, the throat's shape becomes asymmetric, and light passing through experiences frame-dragging, leading to observable Doppler shifts and distortions.
In astrophysics, wormhole throats are studied as potential observational targets: their shadows and lensing signatures could be distinguished from black holes by future telescopes, and they serve as theoretical laboratories for quantum gravity.
A wormhole's throat acts like a gravitational lens so strong that light passing through it can create multiple images of the same background star, and the throat itself can appear as a bright ring — sometimes even brighter than a black hole's shadow.
















