Where is it now
- Distance from Sun
- 1.052 AU
- True anomaly
- 153.22°
- Distance from Earth
- 0.775 AU
- As of
- 17 October 2026
Two-body Kepler propagation — accurate to ~0.1% for major planets over decades, less so for highly-perturbed bodies. Use JPL Horizons for high precision.
In the sky
- Right ascension
- 18h 30m 23s
- Declination
- -22° 34′ 05″
- Constellation
- Sagittarius
- Distance from Earth
- 0.78 AU
- Elongation from the Sun
- 71.73° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
From your location
See how high it is right now, whether it is up after civil twilight, and when it rises and sets where you are.
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Two-body approximation, good to about a degree for the planets — enough to find the constellation and know whether it is up.
Orbital elements
- Semi-major axis
- 0.819 AU
- Eccentricity
- 0.3634
- Inclination
- 0.58°
- Orbital period
- 270.8 days
- Perihelion
- 0.521 AU
- Aphelion
- 1.117 AU
- Longitude of ascending node
- 221.44°
- Argument of periapsis
- 325.34°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.3 LD
- 0.0007 AU
- Tisserand (Jupiter)
- 7.092
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 26
- Data arc
- 2 days
- First observed
- 6 November 2021
- Last observed
- 8 November 2021
- Residual RMS
- 0.28 ″
- Solution · Otto Matic
- 11 November 2021
Visual & observation
- Absolute magnitude (H)
- 30.59
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 142 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-04-16 20:05 UTC close approach of 2021 VN3. Catalogue miss distance 184.1 LD · 7.08 × 10⁷ km. The curve is the geocentric path from 2027-04-13 to 2027-04-19, with a mark at UTC midnights and an arrow for the direction of motion. The circle is the Moon’s mean orbit; the Moon is plotted at closest approach. A ray shows the Sun’s direction. The labelled distance is the full separation. The drawn radius is the part that lies in the ecliptic plane. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2027-04-16 20:05:00 | Earth | 0.4731 AU | 184.1 LD | 17.7 km/s |
| 2027-10-30 17:39:00 | Earth | 0.3896 AU | 151.6 LD | 21.6 km/s |
| 2029-05-21 19:25:00 | Venus | 0.05 AU | 19.4 LD | 10.7 km/s |
| 2029-09-05 08:51:00 | Earth | 0.4627 AU | 180.1 LD | 24 km/s |
| 2030-03-27 00:29:00 | Earth | 0.4761 AU | 185.3 LD | 18.3 km/s |
| 2032-08-28 19:16:00 | Earth | 0.2772 AU | 107.9 LD | 17.9 km/s |
| 2033-03-06 20:19:00 | Earth | 0.461 AU | 179.4 LD | 17.3 km/s |
| 2035-08-24 09:18:00 | Earth | 0.0943 AU | 36.7 LD | 12 km/s |
| 2036-02-14 20:43:00 | Earth | 0.4265 AU | 166.0 LD | 14.7 km/s |
| 2038-09-01 14:50:00 | Earth | 0.065 AU | 25.3 LD | 7.5 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB