The strong consensus against a 100-kiloton meteor strike in 2026 reflects the low annual frequency of such impacts, with objects energetic enough to produce that yield (roughly 10–20 meters across) striking Earth only sporadically and without any detected near-Earth objects on collision courses according to ongoing NASA CNEOS tracking. Recent increases in reported fireballs have been attributed to improved detection of smaller, non-hazardous bolides rather than a shift in larger asteroid populations, consistent with historical records showing events of this magnitude occur far less often than city-killer-scale impacts. Continuous orbital surveys and refined impact probability models continue to show no elevated risk through year-end, though an undetected object or unexpected orbital perturbation remains the primary low-probability scenario that could alter outcomes before resolution.