Where is it now
- Distance from Sun
- 0.504 AU
- True anomaly
- 94.67°
- Distance from Earth
- 0.736 AU
- As of
- 15 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
- 15h 20m 24s
- Declination
- -01° 37′ 29″
- Constellation
- Serpens
- Distance from Earth
- 0.72 AU
- Elongation from the Sun
- 29.56° — 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
- 0.644 AU
- Eccentricity
- 0.4997
- Inclination
- 24.47°
- Orbital period
- 188.9 days
- Perihelion
- 0.322 AU
- Aphelion
- 0.966 AU
- Longitude of ascending node
- 235.04°
- Argument of periapsis
- 11.17°
- Epoch · J2000
- 2461200.5
- Orbit class · IEO
- Atira (interior-Earth object)
- Earth MOID · 14.6 LD
- 0.0375 AU
- Tisserand (Jupiter)
- 8.632
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 48
- Data arc
- 9.87 years
- First observed
- 17 January 2015
- Last observed
- 1 December 2024
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 7 August 2025
Visual & observation
- Absolute magnitude (H)
- 20.46
Discovery & classification
Close approaches 52 on record
Top-down view of the ecliptic, Earth at the centre, for the 2038-11-26 18:43 UTC close approach of 2023 WK3. Catalogue miss distance 62.2 LD · 2.39 × 10⁷ km. The curve is the geocentric path from 2038-11-23 to 2038-11-29, 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 |
|---|---|---|---|---|
| 2038-11-26 18:43:00 | Earth | 0.1599 AU | 62.2 LD | 14.6 km/s |
| 2039-11-20 01:13:00 | Earth | 0.0376 AU | 14.7 LD | 14.2 km/s |
| 2040-11-18 01:29:00 | Earth | 0.1647 AU | 64.1 LD | 17.7 km/s |
| 2053-11-27 16:59:00 | Earth | 0.1848 AU | 71.9 LD | 15 km/s |
| 2054-11-20 20:42:00 | Earth | 0.0501 AU | 19.5 LD | 13.9 km/s |
| 2055-11-18 14:13:00 | Earth | 0.1339 AU | 52.1 LD | 16.9 km/s |
| 2069-11-22 09:19:00 | Earth | 0.0807 AU | 31.4 LD | 13.8 km/s |
| 2070-11-18 08:52:00 | Earth | 0.0931 AU | 36.2 LD | 15.8 km/s |
| 2084-11-24 05:27:00 | Earth | 0.1168 AU | 45.4 LD | 14 km/s |
| 2085-11-18 14:45:00 | Earth | 0.0563 AU | 21.9 LD | 14.9 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