Where is it now
- Distance from Sun
- 0.932 AU
- True anomaly
- 232.03°
- Distance from Earth
- 0.856 AU
- As of
- 19 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 02m 37s
- Declination
- +16° 27′ 54″
- Constellation
- Leo
- Distance from Earth
- 0.86 AU
- Elongation from the Sun
- 59.83° — 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
- 0.84 AU
- Eccentricity
- 0.2619
- Inclination
- 11.37°
- Orbital period
- 281.1 days
- Perihelion
- 0.62 AU
- Aphelion
- 1.06 AU
- Longitude of ascending node
- 59.62°
- Argument of periapsis
- 147.54°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.6 LD
- 0.0119 AU
- Tisserand (Jupiter)
- 6.956
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 36
- Data arc
- 5 days
- First observed
- 19 November 2022
- Last observed
- 24 November 2022
- Residual RMS
- 0.57 ″
- Solution · Otto Matic
- 25 December 2022
Visual & observation
- Absolute magnitude (H)
- 27.44
Discovery & classification
Close approaches 120 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-05-10 00:41 UTC close approach of 2022 WL2. Catalogue miss distance 148.2 LD · 5.7 × 10⁷ km. The curve is the geocentric path from 2029-05-07 to 2029-05-13, 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 |
|---|---|---|---|---|
| 2029-05-10 00:41:00 | Earth | 0.3809 AU | 148.2 LD | 14.1 km/s |
| 2029-11-18 06:51:00 | Earth | 0.4194 AU | 163.2 LD | 20.3 km/s |
| 2032-07-15 08:27:00 | Earth | 0.2907 AU | 113.1 LD | 7.8 km/s |
| 2032-11-20 13:01:00 | Earth | 0.0402 AU | 15.6 LD | 7.6 km/s |
| 2035-09-22 10:04:00 | Earth | 0.3213 AU | 125.1 LD | 14.5 km/s |
| 2036-03-20 06:43:00 | Earth | 0.3856 AU | 150.0 LD | 12.4 km/s |
| 2039-05-20 04:07:00 | Earth | 0.371 AU | 144.4 LD | 13.6 km/s |
| 2039-11-21 20:11:00 | Earth | 0.3373 AU | 131.3 LD | 17.7 km/s |
| 2042-11-05 01:29:00 | Earth | 0.1118 AU | 43.5 LD | 7.2 km/s |
| 2045-09-24 22:24:00 | Earth | 0.412 AU | 160.3 LD | 17.9 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