Where is it now
- Distance from Sun
- 0.985 AU
- True anomaly
- 254.06°
- Distance from Earth
- 0.998 AU
- As of
- 24 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 26m 18s
- Declination
- +16° 30′ 34″
- Constellation
- Leo
- Distance from Earth
- 1 AU
- Elongation from the Sun
- 59.28° — near the Sun — look low at dusk or dawn
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
- 0.967 AU
- Eccentricity
- 0.1699
- Inclination
- 14.22°
- Orbital period
- 347.4 days
- Perihelion
- 0.803 AU
- Aphelion
- 1.131 AU
- Longitude of ascending node
- 65.63°
- Argument of periapsis
- 132.67°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 24.9 LD
- 0.0641 AU
- Tisserand (Jupiter)
- 6.204
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 28
- Data arc
- 10 days
- First observed
- 21 November 2022
- Last observed
- 1 December 2022
- Residual RMS
- 0.53 ″
- Solution · Otto Matic
- 1 December 2022
Visual & observation
- Absolute magnitude (H)
- 23.89
Discovery & classification
Close approaches 68 on record
Top-down view of the ecliptic, Earth at the centre, for the 2039-08-11 04:39 UTC close approach of 2022 WH4. Catalogue miss distance 176.6 LD · 6.79 × 10⁷ km. The curve is the geocentric path from 2039-08-08 to 2039-08-14, 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 |
|---|---|---|---|---|
| 2028-12-26 20:26:00 | Venus | 0.106 AU | 41.2 LD | 7.2 km/s |
| 2039-06-10 18:41:00 | Venus | 0.123 AU | 47.9 LD | 7.7 km/s |
| 2039-08-11 04:39:00 | Earth | 0.4539 AU | 176.6 LD | 17.8 km/s |
| 2040-07-14 18:45:00 | Earth | 0.2248 AU | 87.5 LD | 11 km/s |
| 2041-05-31 22:02:00 | Earth | 0.1667 AU | 64.9 LD | 9.3 km/s |
| 2041-10-31 03:50:00 | Earth | 0.2239 AU | 87.1 LD | 7.7 km/s |
| 2042-04-09 05:01:00 | Earth | 0.2605 AU | 101.4 LD | 8.8 km/s |
| 2042-12-06 02:23:00 | Earth | 0.0652 AU | 25.4 LD | 8.6 km/s |
| 2043-12-07 22:07:00 | Earth | 0.2961 AU | 115.2 LD | 15.1 km/s |
| 2059-08-02 01:24:00 | Earth | 0.3487 AU | 135.7 LD | 14.6 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