Where is it now
- Distance from Sun
- 0.435 AU
- True anomaly
- 34.68°
- Distance from Earth
- 1.364 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
- 14h 17m 10s
- Declination
- -07° 53′ 11″
- Constellation
- Virgo
- Distance from Earth
- 1.36 AU
- Elongation from the Sun
- 12.06° — too close to the Sun to observe
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
- 0.799 AU
- Eccentricity
- 0.4871
- Inclination
- 30.71°
- Orbital period
- 260.7 days
- Perihelion
- 0.41 AU
- Aphelion
- 1.188 AU
- Longitude of ascending node
- 209.3°
- Argument of periapsis
- 358.68°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 74.6 LD
- 0.1917 AU
- Tisserand (Jupiter)
- 7.103
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 548
- Data arc
- 22.84 years
- First observed
- 31 October 2002
- Last observed
- 2 September 2025
- Residual RMS
- 0.39 ″
- Solution · Otto Matic
- 3 September 2025
Physical properties
- Rotation period
- 2.56 hours
Visual & observation
- Absolute magnitude (H)
- 19.11
Discovery & classification
- Discovered by
- LINEAR
- Discovery date
- 31 October 2002
- Discovery site
- Socorro
Also known as 2002 UA31
Close approaches 97 on record
Top-down view of the ecliptic, Earth at the centre, for the 2047-10-16 21:19 UTC close approach of 338292. Catalogue miss distance 77.7 LD · 2.99 × 10⁷ km. The curve is the geocentric path from 2047-10-13 to 2047-10-19, 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. 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 |
|---|---|---|---|---|
| 2032-06-25 09:08:00 | Merc | 0.0573 AU | 22.3 LD | 34.6 km/s |
| 2032-06-25 09:08:00 | Mercury | 0.0573 AU | 22.3 LD | 34.6 km/s |
| 2033-03-12 12:40:00 | Mercury | 0.0314 AU | 12.2 LD | 35.6 km/s |
| 2033-03-12 12:40:00 | Merc | 0.0314 AU | 12.2 LD | 35.6 km/s |
| 2047-10-16 21:19:00 | Earth | 0.1998 AU | 77.7 LD | 16.6 km/s |
| 2052-06-20 17:07:00 | Merc | 0.0394 AU | 15.3 LD | 34.7 km/s |
| 2052-06-20 17:07:00 | Mercury | 0.0394 AU | 15.3 LD | 34.7 km/s |
| 2052-10-16 23:51:00 | Earth | 0.1982 AU | 77.1 LD | 16.6 km/s |
| 2053-03-07 23:55:00 | Merc | 0.0489 AU | 19.0 LD | 36.3 km/s |
| 2053-03-07 23:55:00 | Mercury | 0.0489 AU | 19.0 LD | 36.3 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB