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

Asteroids on 2007-05-02

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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 SF77) 118.7 – 265.5
≈ the Great Pyramid
No 79,178
64 times the speed of sound
round the Earth in 30 minutes
73,143,822 km
190 LD
(2011 BA12) 84.1 – 187.9
≈ a football pitch
No 67,871
55 times the speed of sound
round the Earth in 35 minutes
66,647,456 km
173 LD
(2012 HL31) 86.8 – 194.1
≈ a football pitch
No 42,386
34 times the speed of sound
round the Earth in 57 minutes
31,751,857 km
82.6 LD
(2013 HJ19) 133.2 – 297.9
≈ the Great Pyramid
No 68,550
56 times the speed of sound
round the Earth in 35 minutes
44,303,023 km
115 LD
(2013 JE29) 50.9 – 113.8
≈ a football pitch
No 100,204
81 times the speed of sound
round the Earth in 24 minutes
74,792,231 km
195 LD
(2013 YR2) 38.4 – 85.9
≈ an airliner's wingspan
No 27,442
22 times the speed of sound
round the Earth in 88 minutes
17,073,359 km
44.4 LD
routine about 138 times a year
(2015 CS) 13.9 – 31.2
≈ the Chelyabinsk object
No 45,049
36 times the speed of sound
round the Earth in 53 minutes
21,645,874 km
56.3 LD
(2016 UW80) 43.9 – 98.2
≈ an airliner's wingspan
No 24,109
20 times the speed of sound
round the Earth in 1.7 hours
33,966,122 km
88.4 LD
(2016 VZ1) 16.0 – 35.8
≈ the Chelyabinsk object
No 44,458
36 times the speed of sound
round the Earth in 54 minutes
13,624,159 km
35.4 LD
routine about 138 times a year
(2017 WJ1) 44.1 – 98.6
≈ an airliner's wingspan
No 37,150
30 times the speed of sound
round the Earth in 65 minutes
56,981,499 km
148 LD
(2019 HN4) 5.1 – 11.3
≈ a city bus
No 66,783
54 times the speed of sound
round the Earth in 36 minutes
65,688,183 km
171 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.