Where is it now
- Distance from Sun
- 1.102 AU
- True anomaly
- 147.96°
- Distance from Earth
- 1.035 AU
- As of
- 22 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
- 09h 50m 48s
- Declination
- +17° 53′ 27″
- Constellation
- Leo
- Distance from Earth
- 1.04 AU
- Elongation from the Sun
- 65.71° — 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
- 0.939 AU
- Eccentricity
- 0.2254
- Inclination
- 9.65°
- Orbital period
- 332.3 days
- Perihelion
- 0.727 AU
- Aphelion
- 1.151 AU
- Longitude of ascending node
- 62.07°
- Argument of periapsis
- 238.47°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 5.1 LD
- 0.0131 AU
- Tisserand (Jupiter)
- 6.358
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 16
- Data arc
- 3 days
- First observed
- 21 November 2024
- Last observed
- 24 November 2024
- Residual RMS
- 0.55 ″
- Solution · Otto Matic
- 25 November 2024
Visual & observation
- Absolute magnitude (H)
- 28.17
Discovery & classification
Close approaches 47 on record
Top-down view of the ecliptic, Earth at the centre, for the 2034-11-21 06:59 UTC close approach of 2024 WU3. Catalogue miss distance 22.2 LD · 8.52 × 10⁶ km. The curve is the geocentric path from 2034-11-18 to 2034-11-24, 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 |
|---|---|---|---|---|
| 2034-09-17 01:20:00 | Venus | 0.0865 AU | 33.7 LD | 5.5 km/s |
| 2034-11-21 06:59:00 | Earth | 0.0569 AU | 22.2 LD | 9.9 km/s |
| 2036-05-03 05:27:00 | Earth | 0.1774 AU | 69.0 LD | 7.3 km/s |
| 2036-06-03 18:02:00 | Venus | 0.0888 AU | 34.5 LD | 9.2 km/s |
| 2044-11-24 09:22:00 | Earth | 0.1896 AU | 73.8 LD | 13.7 km/s |
| 2055-12-23 05:29:00 | Earth | 0.1898 AU | 73.9 LD | 6.5 km/s |
| 2057-03-27 11:24:00 | Earth | 0.1966 AU | 76.5 LD | 12.2 km/s |
| 2057-07-01 19:04:00 | Venus | 0.1462 AU | 56.9 LD | 10.6 km/s |
| 2059-03-16 04:01:00 | Venus | 0.0556 AU | 21.7 LD | 5.3 km/s |
| 2065-11-25 01:18:00 | Earth | 0.0884 AU | 34.4 LD | 6.7 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