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

Asteroids on 2017-10-20

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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
500136 (2012 CO46) 71.5 – 160.0
≈ a football pitch
No 6,936
6 times the speed of sound
round the Earth in 5.8 hours
20,519,546 km
53.4 LD
(2014 UR) 12.7 – 28.4
≈ the Chelyabinsk object
No 15,983
13 times the speed of sound
round the Earth in 2.5 hours
9,509,676 km
24.7 LD
routine about 57 times a year
(2016 UA6) 18.4 – 41.1
≈ the Chelyabinsk object
No 67,687
55 times the speed of sound
round the Earth in 36 minutes
64,173,021 km
167 LD
(2017 SH14) 35.0 – 78.4
≈ an airliner's wingspan
No 24,716
20 times the speed of sound
round the Earth in 1.6 hours
5,894,936 km
15.3 LD
routine about 58 times a year
(2017 SY20) 36.0 – 80.5
≈ an airliner's wingspan
No 25,839
21 times the speed of sound
round the Earth in 1.6 hours
7,261,335 km
18.9 LD
routine about 58 times a year
(2017 TO2) 51.6 – 115.4
≈ a football pitch
No 49,262
40 times the speed of sound
round the Earth in 49 minutes
5,339,089 km
13.9 LD
routine about 24 times a year
(2017 UG) 8.4 – 18.8
≈ a city bus
No 38,072
31 times the speed of sound
round the Earth in 63 minutes
1,639,716 km
4.27 LD
routine about 15 times a year
(2017 UP) 16.0 – 35.8
≈ the Chelyabinsk object
No 51,534
42 times the speed of sound
round the Earth in 47 minutes
2,524,012 km
6.57 LD
routine about 25 times a year
(2017 UJ2) 1.8 – 3.9
≈ a car
No 30,539
25 times the speed of sound
round the Earth in 79 minutes
17,897 km
0.05 LD — closer than the Moon
occasional about 2 times a year
(2017 UT2) 32.0 – 71.5
≈ an airliner's wingspan
No 22,614
18 times the speed of sound
round the Earth in 1.8 hours
14,166,810 km
36.9 LD
routine about 138 times a year
(2017 UN5) 8.0 – 17.9
≈ a city bus
No 26,246
21 times the speed of sound
round the Earth in 1.5 hours
3,132,693 km
8.15 LD
routine about 23 times a year
(2017 UA45) 16.0 – 35.8
≈ the Chelyabinsk object
No 15,293
12 times the speed of sound
round the Earth in 2.6 hours
7,142,767 km
18.6 LD
routine about 58 times a year
(2017 UL52) 5.8 – 13.1
≈ a city bus
No 22,043
18 times the speed of sound
round the Earth in 1.8 hours
1,541,802 km
4.01 LD
routine about 15 times a year
(2018 GS1) 80.6 – 180.3
≈ a football pitch
No 36,163
29 times the speed of sound
round the Earth in 66 minutes
13,231,865 km
34.4 LD
routine about 101 times a year
(2019 DV) 88.0 – 196.8
≈ a football pitch
No 75,564
61 times the speed of sound
round the Earth in 32 minutes
69,420,896 km
181 LD
(2019 RF1) 4.6 – 10.3
≈ a city bus
No 62,511
51 times the speed of sound
round the Earth in 38 minutes
61,486,855 km
160 LD
(2019 UW6) 12.7 – 28.4
≈ the Chelyabinsk object
No 43,586
35 times the speed of sound
round the Earth in 55 minutes
10,082,515 km
26.2 LD
routine about 57 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.