Where is it now
- Distance from Sun
- 1.041 AU
- True anomaly
- 194.86°
- Distance from Earth
- 1.719 AU
- As of
- 15 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
- 11h 28m 56s
- Declination
- +06° 56′ 58″
- Constellation
- Leo
- Distance from Earth
- 1.71 AU
- Elongation from the Sun
- 33.35° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
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
- 0.732 AU
- Eccentricity
- 0.463
- Inclination
- 9.06°
- Orbital period
- 228.6 days
- Perihelion
- 0.393 AU
- Aphelion
- 1.071 AU
- Longitude of ascending node
- 101.38°
- Argument of periapsis
- 201.68°
- Epoch · J2000
- 2459219.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.3 LD
- 0.0111 AU
- Tisserand (Jupiter)
- 7.768
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 21
- Data arc
- 2 days
- First observed
- 4 January 2021
- Last observed
- 6 January 2021
- Residual RMS
- 0.41 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 26.7
Discovery & classification
Close approaches 69 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-02-14 17:41 UTC close approach of 2021 AB1. Catalogue miss distance 114.1 LD · 4.39 × 10⁷ km. The curve is the geocentric path from 2028-02-11 to 2028-02-17, 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. At closest approach the object is north of the ecliptic. 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 |
|---|---|---|---|---|
| 2028-02-14 17:41:00 | Earth | 0.2933 AU | 114.1 LD | 20 km/s |
| 2028-11-17 17:40:00 | Merc | 0.0986 AU | 38.4 LD | 28.4 km/s |
| 2028-11-17 17:40:00 | Mercury | 0.0986 AU | 38.4 LD | 28.4 km/s |
| 2030-12-27 19:48:00 | Earth | 0.0939 AU | 36.5 LD | 14.5 km/s |
| 2032-01-06 11:47:00 | Merc | 0.0813 AU | 31.6 LD | 25.9 km/s |
| 2032-01-06 11:47:00 | Mercury | 0.0813 AU | 31.6 LD | 25.9 km/s |
| 2033-02-16 03:42:00 | Earth | 0.2233 AU | 86.9 LD | 17.2 km/s |
| 2033-11-01 01:38:00 | Venus | 0.1415 AU | 55.1 LD | 23 km/s |
| 2034-06-16 11:15:00 | Venus | 0.083 AU | 32.3 LD | 18.8 km/s |
| 2035-01-29 05:44:00 | Venus | 0.0863 AU | 33.6 LD | 14.8 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