Where is it now
- Distance from Sun
- 1.095 AU
- True anomaly
- 139.6°
- Distance from Earth
- 0.176 AU
- As of
- 20 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
- 05h 37m 57s
- Declination
- +18° 37′ 12″
- Constellation
- Taurus
- Distance from Earth
- 0.18 AU
- Elongation from the Sun
- 123.41° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.906 AU
- Eccentricity
- 0.5147
- Inclination
- 8.8°
- Orbital period
- 315.1 days
- Perihelion
- 0.44 AU
- Aphelion
- 1.373 AU
- Longitude of ascending node
- 211.06°
- Argument of periapsis
- 44.69°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 5.2 LD
- 0.0135 AU
- Tisserand (Jupiter)
- 6.449
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 98
- Data arc
- 14.09 years
- First observed
- 30 October 2007
- Last observed
- 3 December 2021
- Residual RMS
- 0.65 ″
- Solution · Otto Matic
- 20 December 2022
Visual & observation
- Absolute magnitude (H)
- 22.13
Discovery & classification
Close approaches 270 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-10-23 09:34 UTC close approach of 2007 US12. Catalogue miss distance 74.5 LD · 2.87 × 10⁷ km. The curve is the geocentric path from 2026-10-20 to 2026-10-26, 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 |
|---|---|---|---|---|
| 2026-10-23 09:34:00 | Earth | 0.1915 AU | 74.5 LD | 11.9 km/s |
| 2027-06-09 12:30:00 | Mercury | 0.0373 AU | 14.5 LD | 20.8 km/s |
| 2027-06-09 12:30:00 | Merc | 0.0373 AU | 14.5 LD | 20.8 km/s |
| 2027-12-29 20:05:00 | Earth | 0.3713 AU | 144.5 LD | 12.1 km/s |
| 2028-03-31 08:13:00 | Earth | 0.4481 AU | 174.4 LD | 15.5 km/s |
| 2029-01-14 08:53:00 | Earth | 0.3963 AU | 154.2 LD | 27.8 km/s |
| 2032-10-19 20:01:00 | Earth | 0.022 AU | 8.6 LD | 16.9 km/s |
| 2033-12-10 20:45:00 | Earth | 0.4083 AU | 158.9 LD | 12.7 km/s |
| 2035-01-24 17:49:00 | Earth | 0.2005 AU | 78.0 LD | 20.2 km/s |
| 2037-10-16 01:19:00 | Merc | 0.0275 AU | 10.7 LD | 21.5 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