The overwhelming 96.9% market-implied probability against a 1-megaton meteor strike in 2026 reflects the absence of any catalogued near-Earth object on a collision trajectory, as confirmed by NASA’s ongoing Planetary Defense Coordination Office surveys and ground-based telescopes. Objects capable of delivering that energy release—roughly 20–50 meters in diameter—are routinely detected years ahead through systematic monitoring of near-Earth asteroids, with no such threat identified for 2026. Historical impact rates indicate events of this scale occur globally only once every few decades on average, yet the current lack of detected candidates and continued refinement of orbital models leave negligible room for an undetected impactor. New data releases from wide-field surveys could still introduce minor adjustments if an object is found late in its approach.