Extensive monitoring by NASA’s Planetary Defense Coordination Office and ground-based surveys has identified no near-Earth objects large enough to produce a 100-kiloton impact (roughly 20–30 meters in diameter) on a collision trajectory for the remainder of 2026. Current orbital catalogs and automated detection systems place the annual probability of an undetected impactor of this size well below 1 percent, consistent with historical rates of roughly one event per several decades. Trader consensus reflects this low baseline risk plus the absence of any recent discoveries or orbital updates that would elevate the chance of an impact before year-end. While an extremely faint, long-period comet on a direct path could theoretically evade detection until late in its approach, such an object would require improbable alignment with observational gaps and would likely trigger rapid follow-up observations if it neared detectable brightness.