A nearby long gamma-ray burst from a merger of compact objects

Gamma-ray bursts (GRBs) are flashes of high-energy radiation arising from energetic cosmic explosions. Bursts of long (greater than two seconds) duration are produced by the core-collapse of massive stars(1), and those of short (less than two seconds) duration by the merger of compact objects, such as two neutron stars(2). A third class of events with hybrid high-energy properties was identified(3), but never conclusively linked to a stellar progenitor. The lack of bright supernovae rules out typical core-collapse explosions(4–6), but their distance scales prevent sensitive searches for direct signatures of a progenitor system. Only tentative evidence for a kilonova has been presented(7,8). Here we report observations of the exceptionally bright GRB 211211A, which classify it as a hybrid event and constrain its distance scale to only 346 megaparsecs. Our measurements indicate that its lower-energy (from ultraviolet to near-infrared) counterpart is powered by a luminous (approximately 10(42) erg per second) kilonova possibly formed in the ejecta of a compact object merger.