Illustration of Earth with several asteroids passing at different distances, one flagged as potentially hazardous

Asteroids on 2008-10-09

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Why is one asteroid “hazardous” when closer ones are not?

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:

  • Its orbit can bring it within 0.05 AU of Earth’s — about 7.5 million km. This is the Minimum Orbit Intersection Distance, the closest the two paths ever come, not the distance on any given pass.
  • It is big enough to matter — absolute magnitude 22.0 or brighter, which is roughly 140 metres across and up. That threshold is a planning convention, not a physical boundary: it is about the size at which an impact could do regional damage. Smaller objects are not harmless, they are simply outside this definition — the Chelyabinsk object of 2013 was around 20 metres and injured about 1,500 people with the shock wave from its airburst, without ever reaching the ground intact.

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
(2006 QQ56) 17.6 – 39.3
≈ the Chelyabinsk object
No 25,346
21 times the speed of sound
round the Earth in 1.6 hours
31,105,716 km
80.9 LD
(2008 GC110) 92.2 – 206.1
≈ a football pitch
No 28,947
23 times the speed of sound
round the Earth in 83 minutes
15,845,675 km
41.2 LD
routine about 101 times a year
(2008 SE) 331.6 – 741.4
≈ the Burj Khalifa
No 19,460
16 times the speed of sound
round the Earth in 2.1 hours
35,662,958 km
92.8 LD
(2008 TL26) 30.5 – 68.2
≈ an airliner's wingspan
No 42,047
34 times the speed of sound
round the Earth in 57 minutes
18,381,244 km
47.8 LD
routine about 138 times a year
(2008 TS26) 0.6 – 1.4
≈ a car
No 56,751
46 times the speed of sound
round the Earth in 42 minutes
12,638 km
0.03 LD — closer than the Moon
occasional about 2 times a year
(2009 VS25) 35.0 – 78.4
≈ an airliner's wingspan
No 26,179
21 times the speed of sound
round the Earth in 1.5 hours
36,213,628 km
94.2 LD
(2013 VL2) 94.3 – 210.9
≈ a football pitch
No 39,679
32 times the speed of sound
round the Earth in 61 minutes
62,097,614 km
162 LD
(2015 FQ) 93.0 – 208.0
≈ a football pitch
No 104,897
85 times the speed of sound
round the Earth in 23 minutes
42,753,078 km
111 LD
(2015 TK143) 160.2 – 358.1
≈ the Great Pyramid
No 58,127
47 times the speed of sound
round the Earth in 41 minutes
32,443,068 km
84.4 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.