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

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(2008 CK70)

Designation: 2008 CK70 · NASA id: 3402249

Estimated diameter: 28 – 62 meters

≈ an airliner's wingspan
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 = 24.9) · JPL Small-Body Database →

Earth impact concern
No identified impact threat
Why?
  • Its closest recorded pass was 1.0 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

530 kilotonnes – 19.8 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 period423.1 days (1.16 years)
Eccentricity.4695633596891876 (0 = circular, closer to 1 = more elongated)
Semi-major axis1.103040228072794 AU
Inclination6.06657249279422° (tilt of its orbit vs. Earth's)
Perihelion distance.5850929527066053 AU (closest approach to the Sun)
Aphelion distance1.620987503438984 AU (farthest from the Sun)
Minimum Orbit Intersection Distance0.00011 AU = 16,489 km
(closest its orbit path ever comes to Earth's, regardless of timing)
Ascending node longitude145.6176678400967°
Argument of perihelion105.9973267689381°
Mean anomaly / motion69.24244011829958° / .8507795584078029°/day
Jupiter Tisserand invariant5.526 (helps distinguish asteroids from comets)
Reference epoch / equinoxJD 2461000.5 / J2000
Orbit determined2021-04-15 01:23:41
Observed2008-01-10 to 2008-02-14 (35 day arc, 87 observations used)
Orbit uncertainty6 (0 = best known, 9 = least certain)

Close Approach History

Every close approach NASA has on record for this object — 40 total.

Why does it pass Earth, Venus and Moon? 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. 29 of them were approaches to Earth, 10 of them were approaches to Venus and 1 of them were approaches to Moon.

This one’s path runs from 0.585 AU at its closest to the Sun out to 1.621 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 423.1 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 (0.0001 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: 2030-02-17

Date Passed near Velocity (km/h) Miss distance
2061-09-30 Earth 76347.72 31,086,770 km
80.9 LD
2061-07-05 Venus 71210.80 15,802,474 km
41.1 LD
2032-10-07 Earth 95069.74 55,758,686 km
145 LD
2031-06-30 Earth 59268.54 61,937,655 km
161 LD
2031-05-19 Venus 53446.08 1,332,379 km
3.47 LD
2030-05-20 Venus 53478.91 6,973,619 km
18.1 LD
2030-02-17 next Earth 46655.01 11,971,864 km
31.1 LD
2024-08-13 Earth 36743.01 44,904,128 km
117 LD
2023-04-10 Earth 44285.99 52,216,005 km
136 LD
2023-01-31 Earth 34448.07 54,735,961 km
142 LD
2017-09-20 Earth 54700.84 8,652,192 km
22.5 LD
2016-05-18 Earth 62471.19 64,150,636 km
167 LD
2015-02-02 Earth 87465.84 44,225,552 km
115 LD
2011-09-07 Venus 64711.69 10,155,368 km
26.4 LD
2010-10-04 Earth 87094.68 45,261,431 km
118 LD
2010-09-06 Venus 43033.16 11,122,077 km
28.9 LD
2009-06-20 Earth 62050.71 63,793,965 km
166 LD
2008-02-15 Earth 55597.70 371,207 km
0.97 LD — closer than the Moon
2008-02-15 Moon 59343.98 741,483 km
1.93 LD
2003-09-25 Earth 70371.81 23,008,049 km
59.9 LD
2002-05-19 Earth 62005.27 63,497,665 km
165 LD
2001-01-27 Earth 100535.10 61,498,134 km
160 LD
1998-10-18 Venus 41361.73 10,919,841 km
28.4 LD
1997-10-07 Venus 47111.26 8,562,738 km
22.3 LD
1996-08-24 Earth 31644.43 39,129,205 km
102 LD
1995-03-20 Earth 32579.22 43,159,018 km
112 LD
1995-02-14 Earth 30400.63 43,061,435 km
112 LD
1990-10-08 Earth 102141.92 65,150,328 km
169 LD
1989-06-21 Earth 60890.77 62,677,713 km
163 LD
1988-02-10 Earth 67595.61 17,242,263 km
44.9 LD
1984-09-21 Venus 43509.72 21,839,519 km
56.8 LD
1983-09-20 Earth 58590.54 9,455,028 km
24.6 LD
1983-08-22 Venus 70888.78 17,916,459 km
46.6 LD
1982-05-06 Earth 58283.93 61,166,535 km
159 LD
1982-01-14 Earth 40120.68 73,169,477 km
190 LD
1976-09-27 Earth 30605.17 52,999,823 km
138 LD
1976-07-31 Earth 42024.37 49,019,745 km
128 LD
1975-02-21 Earth 35174.06 28,829,822 km
75.0 LD
1971-09-16 Venus 52276.45 1,273,283 km
3.31 LD
1970-10-05 Earth 93701.43 53,913,077 km
140 LD

Looked up from NASA's NeoWs API and cached — last refreshed 2026-09-04T21:00:33.506299+00:00.