Where is it now
- Distance from Sun
- 0.842 AU
- True anomaly
- 119.88°
- Distance from Earth
- 0.629 AU
- As of
- 19 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
- 17h 12m 07s
- Declination
- -46° 25′ 41″
- Constellation
- Ara
- Distance from Earth
- 0.63 AU
- Elongation from the Sun
- 57.58° — near the Sun — look low at dusk or dawn
Favours the southern hemisphere; low or below the horizon from far north.
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
- 0.844 AU
- Eccentricity
- 0.5018
- Inclination
- 19.43°
- Orbital period
- 283.2 days
- Perihelion
- 0.42 AU
- Aphelion
- 1.268 AU
- Longitude of ascending node
- 52.27°
- Argument of periapsis
- 177.35°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 79.2 LD
- 0.2036 AU
- Tisserand (Jupiter)
- 6.822
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 113
- Data arc
- 17.04 years
- First observed
- 28 October 2006
- Last observed
- 11 November 2023
- Residual RMS
- 0.51 ″
- Solution · Otto Matic
- 12 November 2023
Visual & observation
- Absolute magnitude (H)
- 21.41
Discovery & classification
- Discovered by
- CSS
- Discovery date
- 28 October 2006
- Discovery site
- Catalina
Also known as 2006 UL185
Close approaches 258 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-11-27 11:39 UTC close approach of 625991. Catalogue miss distance 100.4 LD · 3.86 × 10⁷ km. The curve is the geocentric path from 2027-11-24 to 2027-11-30, 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 |
|---|---|---|---|---|
| 2027-06-16 08:12:00 | Merc | 0.0459 AU | 17.8 LD | 19.8 km/s |
| 2027-06-16 08:12:00 | Mercury | 0.0459 AU | 17.8 LD | 19.8 km/s |
| 2027-11-27 11:39:00 | Earth | 0.2579 AU | 100.4 LD | 13.9 km/s |
| 2030-10-15 21:20:00 | Earth | 0.2303 AU | 89.6 LD | 14.3 km/s |
| 2031-12-10 06:20:00 | Earth | 0.4347 AU | 169.2 LD | 27.1 km/s |
| 2034-06-04 21:23:00 | Mercury | 0.0379 AU | 14.8 LD | 19.5 km/s |
| 2034-06-04 21:23:00 | Merc | 0.0379 AU | 14.8 LD | 19.5 km/s |
| 2034-12-05 23:45:00 | Earth | 0.2317 AU | 90.2 LD | 13.9 km/s |
| 2037-10-24 00:09:00 | Earth | 0.2523 AU | 98.2 LD | 13.8 km/s |
| 2040-10-14 19:03:00 | Earth | 0.4068 AU | 158.3 LD | 25.5 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