2022 UV24 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.65 AU to 1.4 AU from the Sun; one orbit takes 376.5 days. Orbit from the JPL solution of 26 September 2025.
Where is it now
- Distance from Sun
- 1.223 AU
- True anomaly
- 139.22°
- Distance from Earth
- 0.57 AU
- As of
- 3 November 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
- 21h 28m 38s
- Declination
- -10° 03′ 45″
- Constellation
- Capricornus
- Distance from Earth
- 0.58 AU
- Elongation from the Sun
- 99.41° — well clear of the Sun
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
- 1.021 AU
- Eccentricity
- 0.3673
- Inclination
- 20.68°
- Orbital period
- 376.5 days
- Perihelion
- 0.646 AU
- Aphelion
- 1.395 AU
- Longitude of ascending node
- 8.59°
- Argument of periapsis
- 226.57°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 44.5 LD
- 0.1143 AU
- Tisserand (Jupiter)
- 5.87
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 104
- Data arc
- 3.05 years
- First observed
- 7 September 2022
- Last observed
- 24 September 2025
- Residual RMS
- 0.59 ″
- Solution · Otto Matic
- 26 September 2025
Visual & observation
- Absolute magnitude (H)
- 22.29
Discovery & classification
Close approaches 34 on record
Top-down view of the ecliptic, Earth at the centre, for the 2057-09-18 20:54 UTC close approach of 2022 UV24. Catalogue miss distance 52.2 LD · 2.01 × 10⁷ km. The curve is the geocentric path from 2057-09-15 to 2057-09-21, 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 south 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 |
|---|---|---|---|---|
| 2057-09-18 20:54:00 | Earth | 0.1341 AU | 52.2 LD | 13.5 km/s |
| 2058-06-09 08:32:00 | Venus | 0.0347 AU | 13.5 LD | 17.2 km/s |
| 2058-09-19 19:36:00 | Earth | 0.1547 AU | 60.2 LD | 17.2 km/s |
| 2061-07-13 01:45:00 | Venus | 0.0767 AU | 29.8 LD | 14.3 km/s |
| 2090-09-22 02:19:00 | Earth | 0.1898 AU | 73.8 LD | 12.5 km/s |
| 2091-09-19 00:23:00 | Earth | 0.1142 AU | 44.4 LD | 15.2 km/s |
| 2096-07-29 15:17:00 | Venus | 0.0572 AU | 22.3 LD | 18 km/s |
| 2099-09-01 16:27:00 | Venus | 0.0501 AU | 19.5 LD | 14.9 km/s |
| 2124-09-19 17:01:00 | Earth | 0.1291 AU | 50.2 LD | 13.7 km/s |
| 2125-09-20 23:19:00 | Earth | 0.1598 AU | 62.2 LD | 17.5 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