Where is it now
- Distance from Sun
- 1.157 AU
- True anomaly
- 173.17°
- Distance from Earth
- 0.495 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
- 19h 44m 13s
- Declination
- +32° 11′ 56″
- Constellation
- Cygnus
- Distance from Earth
- 0.5 AU
- Elongation from the Sun
- 96.02° — 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
- 0.877 AU
- Eccentricity
- 0.3239
- Inclination
- 25.23°
- Orbital period
- 300 days
- Perihelion
- 0.593 AU
- Aphelion
- 1.161 AU
- Longitude of ascending node
- 241.42°
- Argument of periapsis
- 314.14°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 8.3 LD
- 0.0212 AU
- Tisserand (Jupiter)
- 6.635
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 64
- Data arc
- 5 days
- First observed
- 23 November 2022
- Last observed
- 28 November 2022
- Residual RMS
- 0.35 ″
- Solution · Otto Matic
- 28 November 2022
Visual & observation
- Absolute magnitude (H)
- 25.18
Discovery & classification
Close approaches 63 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-03-28 09:11 UTC close approach of 2022 WU4. Catalogue miss distance 190.0 LD · 7.31 × 10⁷ km. The curve is the geocentric path from 2027-03-25 to 2027-03-31, 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 |
|---|---|---|---|---|
| 2027-03-28 09:11:00 | Earth | 0.4883 AU | 190.0 LD | 18.2 km/s |
| 2027-11-15 12:12:00 | Earth | 0.394 AU | 153.3 LD | 24.5 km/s |
| 2031-06-04 19:05:00 | Earth | 0.3501 AU | 136.3 LD | 18.7 km/s |
| 2031-11-20 14:26:00 | Earth | 0.2143 AU | 83.4 LD | 13.1 km/s |
| 2035-08-12 12:05:00 | Earth | 0.4886 AU | 190.1 LD | 20 km/s |
| 2036-04-20 06:27:00 | Earth | 0.4434 AU | 172.6 LD | 19.8 km/s |
| 2036-11-21 14:20:00 | Earth | 0.1911 AU | 74.4 LD | 19 km/s |
| 2040-06-25 16:45:00 | Earth | 0.3455 AU | 134.5 LD | 17.8 km/s |
| 2040-11-03 06:09:00 | Earth | 0.3628 AU | 141.2 LD | 13.2 km/s |
| 2041-02-23 01:30:00 | Earth | 0.4979 AU | 193.8 LD | 12.2 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