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

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(2016 FB)

Designation: 2016 FB · NASA id: 3747498

Estimated diameter: 49 – 110 meters

≈ a football pitch
That comparison is of size only — what an impact would do depends on speed, angle, composition and where it arrives, none of which follows from width.
(absolute magnitude H = 23.67) · JPL Small-Body Database →

Earth impact concern
No identified impact threat
Why?
  • Its closest recorded pass was 15.0 lunar distances.
  • It is not on NASA/JPL’s Sentry list, which holds every object with a computed chance of impact above zero. Most objects are not on it.
What the four levels mean
  • No identified impact threat — not on any risk list. 98.8% of the objects here.
  • On a monitored risk list — a computed chance above zero, however small. 1.2% of the objects here.
  • Among the highest-ranked — Palermo at or above −2. Two objects worldwide qualify, both studied for decades and both centuries away.
  • Exceptional — Torino 1 or more, or Palermo at or above zero. No object anywhere currently qualifies.

These describe where an object sits in a catalogue, not how dangerous it is. The full ranked list is on the impact risk page.

Energy of motion, if it ever entered the atmosphere

1.4 megatonnes – 51.6 megatonnes of TNT

This is not a forecast. Nothing here says this object will arrive, and almost nothing ever does — what is actually assessed, by people with far better data than this page has, is on the impact risk page. This is simply the kinetic energy such a body would carry, worked out from its size and its usual encounter speed.

The range spans a factor of 37, and it cannot be narrowed. Nobody has weighed this object. Its diameter is inferred from how bright it is under an assumed reflectivity, which carries a fixed factor of 2.24 — and because mass goes as the cube of diameter, that alone becomes a factor of 11. Density is then assumed somewhere between 1,500 and 5,000 kg/m³, from a loose rubble pile to dense rock. Quoting a tighter figure would be invented precision.

Megatonnes do not mean what the word suggests here. Most of this energy is spent high in the atmosphere, not on the ground, and the comparison with weapons misleads badly. The Chelyabinsk body released around 440 kilotonnes in 2013 — this same calculation gives it 166 to 904 — and the damage was broken windows across a city, from the shock wave of an airburst some thirty kilometres up. No crater, and nothing that reached the ground intact.

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.

Orbital Data

Orbit class: APO — Near-Earth asteroid orbits which cross the Earth’s orbit similar to that of 1862 Apollo
a (semi-major axis) > 1.0 AU; q (perihelion) < 1.017 AU

Orbital period507.6 days (1.39 years)
Eccentricity.1848999373215039 (0 = circular, closer to 1 = more elongated)
Semi-major axis1.245306109008256 AU
Inclination19.31366504629602° (tilt of its orbit vs. Earth's)
Perihelion distance1.015049087506543 AU (closest approach to the Sun)
Aphelion distance1.475563130509968 AU (farthest from the Sun)
Minimum Orbit Intersection Distance0.03195 AU = 4,779,188 km
(closest its orbit path ever comes to Earth's, regardless of timing)
Ascending node longitude359.5901607293893°
Argument of perihelion155.6265220291432°
Mean anomaly / motion1.084698215839099° / .7092345698121124°/day
Jupiter Tisserand invariant5.086 (helps distinguish asteroids from comets)
Reference epoch / equinoxJD 2461000.5 / J2000
Orbit determined2021-04-15 16:46:10
Observed2016-03-16 to 2016-03-31 (15 day arc, 163 observations used)
Orbit uncertainty7 (0 = best known, 9 = least certain)

Close Approach History

Every close approach NASA has on record for this object — 52 total.

Why does it pass Earth and Mars? Doesn’t it orbit just one?

It orbits the Sun. Not Earth, and not Venus. The column above does not say what the asteroid goes around — it says which planet a given close approach was to. 48 of them were approaches to Earth and 4 of them were approaches to Mars.

This one’s path runs from 1.015 AU at its closest to the Sun out to 1.476 AU at its farthest. For scale, Venus orbits at about 0.72 AU and Earth at 1.00 AU — so an orbit spanning that range crosses the path of every planet in between, once on the way out and once on the way back.

Crossing a planet’s path is not the same as meeting the planet. Almost every time the asteroid crosses, that planet is somewhere else along its own orbit. A close approach is logged only on the rare occasions when both happen to arrive at the crossing point at roughly the same time — which is why the dates below are scattered rather than regular. This object takes 507.6 days to go round, against Earth’s 365.25, so the two drift in and out of step over years rather than repeating on a neat cycle.

The Minimum Orbit Intersection Distance in the table above (0.0319 AU) is the closest the two paths ever come. The miss distances below are how far apart the two bodies actually were on the day, which is almost always very much larger.

next approach: 2033-10-21

Date Passed near Velocity (km/h) Miss distance
2173-03-08 Earth 45938.32 45,189,473 km
118 LD
2171-02-28 Mars 33206.90 11,479,097 km
29.9 LD
2169-09-15 Earth 40542.30 70,021,703 km
182 LD
2166-03-22 Earth 38694.49 6,139,368 km
16.0 LD
2159-04-08 Earth 59727.30 58,485,245 km
152 LD
2158-10-27 Earth 35856.72 60,131,356 km
156 LD
2151-10-04 Earth 39826.69 64,074,941 km
167 LD
2148-03-08 Earth 45112.67 43,237,643 km
112 LD
2112-11-07 Mars 32886.54 10,123,981 km
26.3 LD
2105-03-02 Earth 54325.35 64,157,048 km
167 LD
2101-09-20 Earth 40529.60 68,021,054 km
177 LD
2098-03-18 Earth 37864.51 7,871,420 km
20.5 LD
2094-08-30 Earth 39210.98 74,687,339 km
194 LD
2091-04-03 Earth 53192.60 45,743,212 km
119 LD
2090-11-02 Earth 34050.54 59,643,533 km
155 LD
2083-10-09 Earth 39157.05 62,513,781 km
163 LD
2080-03-02 Earth 52420.87 60,470,297 km
157 LD
2076-09-18 Earth 40521.90 68,400,316 km
178 LD
2073-03-17 Earth 37819.78 9,280,012 km
24.1 LD
2066-03-31 Earth 50064.43 39,100,080 km
102 LD
2055-02-27 Earth 59591.27 74,745,448 km
194 LD
2048-03-11 Earth 40109.12 27,735,335 km
72.2 LD
2041-03-25 Earth 42081.58 19,021,972 km
49.5 LD
2034-04-09 Earth 64548.76 66,826,124 km
174 LD
2033-10-21 next Earth 36926.71 60,241,128 km
157 LD
2026-10-01 Earth 39904.90 64,412,687 km
168 LD
2023-03-07 Earth 45548.97 44,934,923 km
117 LD
2019-09-14 Earth 40439.61 70,277,400 km
183 LD
2016-03-20 Earth 38608.61 5,770,759 km
15.0 LD
2009-04-05 Earth 58936.62 56,539,051 km
147 LD
2008-10-25 Earth 35840.14 59,526,585 km
155 LD
2001-10-02 Earth 39699.30 63,671,001 km
166 LD
1998-03-06 Earth 46148.69 46,723,871 km
122 LD
1994-09-13 Earth 40417.33 70,295,134 km
183 LD
1991-03-22 Earth 39290.82 8,615,240 km
22.4 LD
1990-08-05 Mars 32583.71 9,127,314 km
23.7 LD
1984-04-08 Earth 64254.77 66,094,762 km
172 LD
1976-09-26 Earth 40205.37 65,240,232 km
170 LD
1973-03-11 Earth 40263.46 28,931,874 km
75.3 LD
1969-09-05 Earth 39954.39 72,696,876 km
189 LD
1966-03-28 Earth 45975.10 29,506,516 km
76.8 LD
1958-10-11 Earth 38654.10 61,205,809 km
159 LD
1955-03-01 Earth 54980.66 66,408,967 km
173 LD
1951-09-19 Earth 40438.36 67,970,260 km
177 LD
1948-03-17 Earth 37766.47 8,724,360 km
22.7 LD
1941-04-02 Earth 53754.50 46,483,435 km
121 LD
1940-10-30 Earth 34552.52 59,024,774 km
154 LD
1933-10-06 Earth 39275.95 62,491,451 km
163 LD
1932-04-09 Mars 31561.16 12,902,053 km
33.6 LD
1930-03-04 Earth 50511.42 57,226,862 km
149 LD
1926-09-16 Earth 40464.29 69,080,703 km
180 LD
1923-03-18 Earth 37944.77 5,952,898 km
15.5 LD

Looked up from NASA's NeoWs API and cached — last refreshed 2026-09-25T12:34:37.234040+00:00.