Because the flag has nothing to do with how close it came on the day. NASA marks an object a Potentially Hazardous Asteroid only if both of these are true of its orbit and its size:
The two terms:
AU — astronomical unit, the average Earth–Sun distance, 149,597,871 km. 0.05 AU is about 7.5 million km.
MOID — minimum orbit intersection distance, the closest the two orbits ever come, whatever the timing.
See the glossary for NEO, PHA and H.
So a large rock passing at 39 million km today can be flagged, because on some future orbit it could come far nearer — while a pebble skimming past at 4 million km is not, because it would never reach the ground.
Three objects that all passed Earth on 30 August 2026 make the point better than any definition:
| Object | Size | Orbit’s closest to Earth’s | Missed by, that day | Flagged |
|---|---|---|---|---|
| 2013 JR28 | 122–272 m | 5.3 M km (0.035 AU) | 39.2 M km | Yes — both tests pass |
| 2012 LE11 | 629–1,406 m | 23.3 M km (0.156 AU) | 26.1 M km | No — orbit never gets near enough |
| 2007 EK | 3.7–8.2 m | 198,000 km (0.0013 AU) | 4.2 M km | No — far too small |
The middle one is five times larger than the flagged one and passed closer on the day, but its path can never come within 23 million km of ours. The last one’s orbit crosses inside the Moon’s distance — nearer than any other object here — and it is still not hazardous, because at a few metres across it would burn up long before it landed.
“Potentially hazardous” is a watchlist criterion, not a prediction. None of these is on a collision course; the label means an object is worth keeping precise track of over the coming centuries.
| Name | Diameter (m) | Hazardous | Velocity (km/h) | Miss distance |
|---|---|---|---|---|
| 499496 (2010 MR87) | 337.7 – 755.2
≈ the Burj Khalifa
|
No | 67,816
55 times the speed of sound round the Earth in 35 minutes |
28,345,945 km 73.7 LD |
| (2008 TX3) | 27.8 – 62.2
≈ an airliner's wingspan
|
No | 60,405
49 times the speed of sound round the Earth in 40 minutes |
65,905,706 km 171 LD |
| (2014 RX22) | 16.8 – 37.5
≈ the Chelyabinsk object
|
No | 46,816
38 times the speed of sound round the Earth in 51 minutes |
37,754,644 km 98.2 LD |
| (2016 FB) | 49.0 – 109.7
≈ a football pitch
|
No | 39,905
32 times the speed of sound round the Earth in 60 minutes |
64,412,687 km 168 LD |
| (2018 LC1) | 27.8 – 62.2
≈ an airliner's wingspan
|
No | 30,362
25 times the speed of sound round the Earth in 79 minutes |
71,893,233 km 187 LD |
| (2019 SD7) | 48.4 – 108.2
≈ a football pitch
|
No | 30,662
25 times the speed of sound round the Earth in 78 minutes |
43,473,504 km 113 LD |
The tag beside a distance says how often an approach at least that close, by an object of that size, appears in 127 years of this archive — a frequency rather than a percentile, because almost every close approach would score in the top few per cent and the scale would say nothing. Approaches beyond 50 lunar distances get no tag, since there is nothing useful to say about them. The counts are a floor: the archive holds the objects known today, and most of the undiscovered ones are small. The ≈ line beside a diameter compares size only. What an impact would do depends on speed, angle, composition and where it arrives, and none of that follows from width — the Chelyabinsk comparison in particular names a body remembered for its airburst, not for how wide it was.