CN HULIANWANG DIGUI 226 and CN HULIANWANG DIGUI 227 were predicted to reach a closest approach of 7.80 km at 2026-10-29 01:55 UTC, at a relative speed of 0.01 km/s. Last computed 29 Oct 01:55 UTC, while the two were flying close together. These two were already within 7.80 km of each other when this was computed and moving apart: they were flying close together rather than crossing paths, so this is their separation at the time shown. Best estimate after the pass, from the orbit data published nearest its time: 36.9 km at 29 Oct 01:33 UTC. Miss distance and time of closest approach are computed by propagating the latest published orbital elements for both objects, and each pass is re-checked every 20 minutes as new element sets are published. See the Satellite Maneuver Tracker for the live picture and space situational awareness for context.
The Two Objects
Where This Happens
At 1049 km this pass sits inside the most congested band in low Earth orbit, home to the debris left by the 2007 ASAT test and the 2009 collision. Objects here stay up for decades: there is too little atmospheric drag to clean the band naturally. Why crowded bands matter →
History Between This Pair
Repeat encounters are common for objects in near-intersecting orbital planes. Each pass is re-screened as fresh element sets arrive; "Final forecast" means the screening still predicted it within 45 minutes of its time, "Not re-confirmed" means later screening stopped finding it.
Forecast Record
These Objects Elsewhere
How These Numbers Are Computed
Miss distance and TCA come from propagating the latest published orbital elements for both objects and searching for the minimum separation over the screening window. Element sets carry kilometre-scale uncertainty, so figures here describe a close pass, not a collision prediction; a change in either object's published elements re-computes the pass automatically. What is a conjunction? → How conjunction assessment works →