2022 UV5 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.85 AU to 1.18 AU from the Sun; one orbit takes 371.1 days. Orbit from the JPL solution of 15 October 2023.
Where is it now
- Distance from Sun
- 1.049 AU
- True anomaly
- 247.68°
- Distance from Earth
- 0.392 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
- 20h 40m 21s
- Declination
- -14° 26′ 42″
- Constellation
- Aquarius
- Distance from Earth
- 0.39 AU
- Elongation from the Sun
- 87.15° — 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
- 1.011 AU
- Eccentricity
- 0.1633
- Inclination
- 9.77°
- Orbital period
- 371.1 days
- Perihelion
- 0.846 AU
- Aphelion
- 1.176 AU
- Longitude of ascending node
- 207.86°
- Argument of periapsis
- 283.79°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 8.0 LD
- 0.0204 AU
- Tisserand (Jupiter)
- 6.005
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 21
- Data arc
- 364 days
- First observed
- 16 October 2022
- Last observed
- 15 October 2023
- Residual RMS
- 0.48 ″
- Solution · Otto Matic
- 15 October 2023
Visual & observation
- Absolute magnitude (H)
- 25.67
Discovery & classification
Close approaches 88 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-03-24 11:00 UTC close approach of 2022 UV5. Catalogue miss distance 58.4 LD · 2.25 × 10⁷ km. The curve is the geocentric path from 2027-03-21 to 2027-03-27, 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 |
|---|---|---|---|---|
| 2027-03-24 11:00:00 | Earth | 0.1501 AU | 58.4 LD | 5.7 km/s |
| 2028-04-18 15:49:00 | Earth | 0.0747 AU | 29.1 LD | 5.9 km/s |
| 2029-05-01 00:23:00 | Earth | 0.0539 AU | 21.0 LD | 7.3 km/s |
| 2030-05-09 08:05:00 | Earth | 0.1388 AU | 54.0 LD | 9.7 km/s |
| 2031-05-16 04:44:00 | Earth | 0.2398 AU | 93.3 LD | 12.4 km/s |
| 2032-05-21 13:07:00 | Earth | 0.3436 AU | 133.7 LD | 15.3 km/s |
| 2033-05-27 08:45:00 | Earth | 0.4477 AU | 174.2 LD | 18.3 km/s |
| 2077-10-11 13:51:00 | Earth | 0.4401 AU | 171.3 LD | 18.4 km/s |
| 2078-10-16 09:00:00 | Earth | 0.3334 AU | 129.7 LD | 15.3 km/s |
| 2079-10-20 23:41:00 | Earth | 0.2266 AU | 88.2 LD | 12.3 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