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

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(2005 VS)

Designation: 2005 VS · NASA id: 3297392

Estimated diameter: 95 – 212 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 = 22.24) · JPL Small-Body Database →

Earth impact concern
No identified impact threat
Why?
  • Its closest recorded pass was 6.4 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

5.0 megatonnes – 185.8 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 period589.7 days (1.61 years)
Eccentricity.2877648695857056 (0 = circular, closer to 1 = more elongated)
Semi-major axis1.376173841536732 AU
Inclination10.14327879135985° (tilt of its orbit vs. Earth's)
Perihelion distance.9801593554996549 AU (closest approach to the Sun)
Aphelion distance1.772188327573809 AU (farthest from the Sun)
Minimum Orbit Intersection Distance0.01721 AU = 2,574,295 km
(closest its orbit path ever comes to Earth's, regardless of timing)
Ascending node longitude227.9352867086025°
Argument of perihelion149.4837142151154°
Mean anomaly / motion164.1249789535363° / .6105118896353529°/day
Jupiter Tisserand invariant4.751 (helps distinguish asteroids from comets)
Reference epoch / equinoxJD 2461000.5 / J2000
Orbit determined2021-04-14 23:09:34
Observed2005-11-03 to 2019-01-01 (4807 day arc, 67 observations used)
Orbit uncertainty0 (0 = best known, 9 = least certain)

Close Approach History

Every close approach NASA has on record for this object — 51 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 3 of them were approaches to Mars.

This one’s path runs from 0.980 AU at its closest to the Sun out to 1.772 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 589.7 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 (0.0172 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.

an approach today (2026-10-17) — next after that: 2034-06-27

Date Passed near Velocity (km/h) Miss distance
2194-08-05 Earth 66117.27 73,004,633 km
190 LD
2189-12-08 Earth 64655.46 61,259,250 km
159 LD
2189-06-21 Earth 27108.37 73,508,571 km
191 LD
2181-11-07 Earth 26809.77 2,445,932 km
6.36 LD
2173-08-09 Earth 57606.66 61,859,955 km
161 LD
2168-12-09 Earth 67326.85 65,002,038 km
169 LD
2160-10-26 Earth 24353.91 10,973,105 km
28.5 LD
2147-12-01 Earth 51407.94 41,326,698 km
108 LD
2147-07-03 Earth 22526.89 64,974,761 km
169 LD
2139-09-03 Earth 32879.56 32,917,545 km
85.6 LD
2126-11-15 Earth 31718.39 9,781,947 km
25.4 LD
2119-01-06 Earth 18701.42 67,812,750 km
176 LD
2118-08-15 Earth 48486.56 50,457,564 km
131 LD
2105-11-11 Earth 28839.44 4,348,797 km
11.3 LD
2097-08-25 Earth 36873.97 37,329,074 km
97.1 LD
2084-12-03 Earth 59489.24 53,398,222 km
139 LD
2084-06-22 Earth 25619.38 70,101,603 km
182 LD
2076-11-06 Earth 26935.50 2,569,401 km
6.68 LD
2069-01-04 Earth 18918.10 68,090,597 km
177 LD
2068-08-12 Earth 48901.49 50,884,081 km
132 LD
2055-11-19 Earth 36725.23 18,318,030 km
47.7 LD
2055-07-24 Earth 11854.04 52,558,841 km
137 LD
2047-08-31 Earth 32634.61 32,849,135 km
85.5 LD
2034-11-30 Earth 54105.05 45,304,987 km
118 LD
2034-06-27 next Earth 23822.02 66,618,884 km
173 LD
2026-10-17 today Earth 24089.74 15,738,548 km
40.9 LD
2018-08-03 Earth 62946.49 68,468,199 km
178 LD
2013-12-05 Earth 65373.15 61,883,764 km
161 LD
2013-06-17 Earth 27389.29 73,792,758 km
192 LD
2005-10-31 Earth 24970.49 7,048,905 km
18.3 LD
1997-08-02 Earth 64316.16 70,237,870 km
183 LD
1992-12-02 Earth 59244.22 52,729,399 km
137 LD
1992-06-22 Earth 25562.42 70,059,219 km
182 LD
1984-09-25 Earth 25747.66 23,346,225 km
60.7 LD
1971-11-23 Earth 42040.79 26,674,171 km
69.4 LD
1971-07-11 Earth 17670.21 57,415,510 km
149 LD
1963-12-18 Earth 16312.49 60,395,479 km
157 LD
1963-08-19 Earth 40965.45 41,638,087 km
108 LD
1950-11-09 Earth 28447.46 3,810,895 km
9.91 LD
1942-12-22 Earth 16568.62 61,631,651 km
160 LD
1942-08-16 Earth 42113.34 42,994,626 km
112 LD
1937-05-15 Mars 21959.63 14,691,926 km
38.2 LD
1929-11-25 Earth 47893.70 35,766,458 km
93.0 LD
1929-07-02 Earth 21415.55 61,994,812 km
161 LD
1926-02-03 Mars 22281.35 14,262,024 km
37.1 LD
1921-10-05 Earth 24612.10 20,289,027 km
52.8 LD
1914-10-26 Mars 22910.82 14,469,355 km
37.6 LD
1913-08-01 Earth 63222.61 68,780,185 km
179 LD
1908-12-05 Earth 67164.35 64,295,317 km
167 LD
1908-06-15 Earth 27917.97 74,757,890 km
194 LD
1900-11-07 Earth 27538.88 2,920,057 km
7.60 LD

Looked up from NASA's NeoWs API and cached — last refreshed 2026-10-12T20:37:49.605898+00:00.