Where is it now
- Distance from Sun
- 2.892 AU
- True anomaly
- 150.31°
- Distance from Earth
- 3.543 AU
- As of
- 11 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
- 10h 16m 08s
- Declination
- -06° 49′ 00″
- Constellation
- Sextans
- Distance from Earth
- 3.54 AU
- Elongation from the Sun
- 43.19° — near the Sun — look low at dusk or dawn
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
- 2.182 AU
- Eccentricity
- 0.6543
- Inclination
- 21.03°
- Orbital period
- 3.22 years
- Perihelion
- 0.754 AU
- Aphelion
- 3.61 AU
- Longitude of ascending node
- 217.48°
- Argument of periapsis
- 135.73°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 40.2 LD
- 0.1032 AU
- Tisserand (Jupiter)
- 3.299
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 2,251
- Data arc
- 24.02 years
- First observed
- 15 March 2002
- Last observed
- 21 March 2026
- Residual RMS
- 0.46 ″
- Solution · Otto Matic
- 22 March 2026
Physical properties
- Rotation period
- 36.4 hours
Visual & observation
- Absolute magnitude (H)
- 15.36
Discovery & classification
- Discovered by
- NEAT
- Discovery date
- 26 December 2003
- Discovery site
- Haleakala
Also known as 2003 YQ117
Close approaches 9 on record
Top-down view of the ecliptic, Earth at the centre, for the 2051-11-06 15:11 UTC close approach of 143947. Catalogue miss distance 47.6 LD · 1.83 × 10⁷ km. The curve is the geocentric path from 2051-11-03 to 2051-11-09, 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 |
|---|---|---|---|---|
| 2029-04-10 04:18:00 | Venus | 0.1126 AU | 43.8 LD | 19.5 km/s |
| 2051-11-06 15:11:00 | Earth | 0.1223 AU | 47.6 LD | 19 km/s |
| 2080-10-28 13:23:00 | Earth | 0.1642 AU | 63.9 LD | 18.2 km/s |
| 2084-01-10 04:13:00 | Venus | 0.1153 AU | 44.9 LD | 19.6 km/s |
| 2138-10-10 05:56:00 | Venus | 0.125 AU | 48.6 LD | 18.5 km/s |
| 2183-11-23 16:53:00 | Earth | 0.1928 AU | 75.0 LD | 23.5 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