Where is it now
- Distance from Sun
- 0.966 AU
- True anomaly
- 221.09°
- Distance from Earth
- 1.425 AU
- As of
- 16 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
- 10h 39m 08s
- Declination
- -03° 09′ 24″
- Constellation
- Sextans
- Distance from Earth
- 1.42 AU
- Elongation from the Sun
- 42.56° — 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
- 0.803 AU
- Eccentricity
- 0.502
- Inclination
- 16.39°
- Orbital period
- 262.9 days
- Perihelion
- 0.4 AU
- Aphelion
- 1.206 AU
- Longitude of ascending node
- 218.27°
- Argument of periapsis
- 37.64°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.7 LD
- 0.0018 AU
- Tisserand (Jupiter)
- 7.131
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 110
- Data arc
- 2 days
- First observed
- 31 October 2022
- Last observed
- 2 November 2022
- Residual RMS
- 0.4 ″
- Solution · Otto Matic
- 13 November 2022
Visual & observation
- Absolute magnitude (H)
- 28.14
Discovery & classification
Close approaches 213 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-11-05 18:51 UTC close approach of 2022 UK24. Catalogue miss distance 82.2 LD · 3.16 × 10⁷ km. The curve is the geocentric path from 2027-11-02 to 2027-11-08, 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 |
|---|---|---|---|---|
| 2026-12-10 16:05:00 | Merc | 0.0145 AU | 5.7 LD | 29 km/s |
| 2026-12-10 16:05:00 | Mercury | 0.0145 AU | 5.7 LD | 29 km/s |
| 2027-08-30 06:39:00 | Mercury | 0.0265 AU | 10.3 LD | 30.7 km/s |
| 2027-08-30 06:39:00 | Merc | 0.0265 AU | 10.3 LD | 30.7 km/s |
| 2027-11-05 18:51:00 | Earth | 0.2112 AU | 82.2 LD | 22.2 km/s |
| 2028-05-19 00:48:00 | Mercury | 0.0492 AU | 19.1 LD | 32.7 km/s |
| 2028-05-19 00:48:00 | Merc | 0.0492 AU | 19.1 LD | 32.7 km/s |
| 2029-02-05 21:38:00 | Mercury | 0.0736 AU | 28.6 LD | 34.9 km/s |
| 2029-02-05 21:38:00 | Merc | 0.0736 AU | 28.6 LD | 34.9 km/s |
| 2029-03-30 05:11:00 | Venus | 0.1458 AU | 56.7 LD | 18.9 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