NASA's Swift Observatory has documented a nomadic supermassive black hole disintegrating a star located over 30,000 light-years from its galactic core. This black hole, approximately one million times heavier than the Sun, emitted a burst that briefly glowed with the intensity of about 10 billion suns, reaching temperatures close to 54,000 degrees Fahrenheit. The phenomenon was initially detected in November 2025 by the Zwicky Transient Facility in California, with results published on July 27, 2026. Researchers indicate that upcoming surveys may reveal numerous additional concealed, wandering black holes.
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