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

Asteroids on 2018-10-19

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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
(2003 LN6) 30.4 – 67.9
≈ an airliner's wingspan
No 29,998
24 times the speed of sound
round the Earth in 80 minutes
43,436,024 km
113 LD
(2006 TD) 88.0 – 196.8
≈ a football pitch
No 66,659
54 times the speed of sound
round the Earth in 36 minutes
54,306,302 km
141 LD
(2009 UQ5) 38.4 – 85.9
≈ an airliner's wingspan
No 31,547
26 times the speed of sound
round the Earth in 76 minutes
34,516,219 km
89.8 LD
(2009 UC19) 24.2 – 54.2
≈ an airliner's wingspan
No 35,758
29 times the speed of sound
round the Earth in 67 minutes
6,898,805 km
17.9 LD
routine about 58 times a year
(2010 FA81) 87.2 – 195.0
≈ a football pitch
No 33,230
27 times the speed of sound
round the Earth in 72 minutes
60,139,555 km
156 LD
(2014 TG17) 86.0 – 192.3
≈ a football pitch
No 37,551
30 times the speed of sound
round the Earth in 64 minutes
22,598,266 km
58.8 LD
(2014 WN4) 58.2 – 130.0
≈ a football pitch
No 65,251
53 times the speed of sound
round the Earth in 37 minutes
67,487,155 km
176 LD
(2015 YS) 18.4 – 41.1
≈ the Chelyabinsk object
No 22,996
19 times the speed of sound
round the Earth in 1.7 hours
72,245,469 km
188 LD
(2016 FB12) 16.8 – 37.5
≈ the Chelyabinsk object
No 27,227
22 times the speed of sound
round the Earth in 88 minutes
69,720,802 km
181 LD
(2016 GH135) 101.1 – 226.0
≈ the Great Pyramid
No 43,606
35 times the speed of sound
round the Earth in 55 minutes
21,386,185 km
55.6 LD
(2017 GM6) 16.8 – 37.5
≈ the Chelyabinsk object
No 29,022
24 times the speed of sound
round the Earth in 83 minutes
27,878,680 km
72.5 LD
(2017 UF1) 12.7 – 28.4
≈ the Chelyabinsk object
No 66,948
54 times the speed of sound
round the Earth in 36 minutes
30,966,858 km
80.6 LD
(2018 EC1) 15.3 – 34.2
≈ the Chelyabinsk object
No 27,633
22 times the speed of sound
round the Earth in 87 minutes
57,723,538 km
150 LD
(2018 SB1) 60.9 – 136.2
≈ a football pitch
No 18,321
15 times the speed of sound
round the Earth in 2.2 hours
17,256,079 km
44.9 LD
routine about 101 times a year
(2018 TJ3) 29.1 – 65.2
≈ an airliner's wingspan
No 32,249
26 times the speed of sound
round the Earth in 75 minutes
16,148,381 km
42.0 LD
routine about 138 times a year
(2018 TA5) 53.0 – 118.6
≈ a football pitch
No 82,355
67 times the speed of sound
round the Earth in 29 minutes
9,579,012 km
24.9 LD
routine about 101 times a year
(2018 TF6) 14.6 – 32.7
≈ the Chelyabinsk object
No 21,473
17 times the speed of sound
round the Earth in 1.9 hours
8,469,163 km
22.0 LD
routine about 138 times a year
(2018 UA) 2.4 – 5.4
≈ a car
No 50,926
41 times the speed of sound
round the Earth in 47 minutes
13,672 km
0.04 LD — closer than the Moon
occasional about 2 times a year
(2018 UR1) 53.0 – 118.6
≈ a football pitch
No 116,815
95 times the speed of sound
round the Earth in 21 minutes
24,210,231 km
63.0 LD
(2018 VG1) 515.9 – 1153.6
≈ the Burj Khalifa
No 100,001
81 times the speed of sound
round the Earth in 24 minutes
25,873,246 km
67.3 LD
(2019 GK3) 3.3 – 7.5
≈ a city bus
No 9,848
8 times the speed of sound
round the Earth in 4.1 hours
21,408,819 km
55.7 LD
(2019 HM) 17.6 – 39.3
≈ the Chelyabinsk object
No 11,209
9 times the speed of sound
round the Earth in 3.6 hours
2,415,481 km
6.28 LD
routine about 25 times a year

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.