Where is it now
- Distance from Sun
- 2.263 AU
- True anomaly
- 199.27°
- Distance from Earth
- 2.654 AU
- As of
- 11 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 20m 11s
- Declination
- -08° 34′ 07″
- Constellation
- Hydra
- Distance from Earth
- 2.65 AU
- Elongation from the Sun
- 56.88° — 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
- 1.505 AU
- Eccentricity
- 0.7026
- Inclination
- 29.18°
- Orbital period
- 674.4 days
- Perihelion
- 0.448 AU
- Aphelion
- 2.563 AU
- Longitude of ascending node
- 235.43°
- Argument of periapsis
- 49.76°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 61.8 LD
- 0.1587 AU
- Tisserand (Jupiter)
- 4.126
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 2,489
- Data arc
- 39.24 years
- First observed
- 30 November 1986
- Last observed
- 27 February 2026
- Residual RMS
- 0.46 ″
- Solution · Otto Matic
- 18 September 2026
Physical properties
- Rotation period
- 2.38 hours
Visual & observation
- Absolute magnitude (H)
- 15.67
Discovery & classification
- Discovered by
- Maury, A.
- Discovery date
- 27 November 1986
- Discovery site
- Palomar
Also known as 3838 · 1986 WA
Close approaches 13 on record
Top-down view of the ecliptic, Earth at the centre, for the 2034-11-07 15:09 UTC close approach of Epona. Catalogue miss distance 77.0 LD · 2.96 × 10⁷ km. The curve is the geocentric path from 2034-11-04 to 2034-11-10, 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 north 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 |
|---|---|---|---|---|
| 2034-11-07 15:09:00 | Earth | 0.198 AU | 77.0 LD | 29.8 km/s |
| 2081-02-20 07:52:00 | Mars | 0.0939 AU | 36.5 LD | 19.1 km/s |
| 2119-10-31 20:08:00 | Earth | 0.1996 AU | 77.7 LD | 23.3 km/s |
| 2143-10-31 21:32:00 | Earth | 0.1986 AU | 77.3 LD | 23.3 km/s |
| 2180-10-29 14:30:00 | Mars | 0.0875 AU | 34.1 LD | 19.5 km/s |
| 2184-03-29 03:12:00 | Merc | 0.0714 AU | 27.8 LD | 33.8 km/s |
| 2184-03-29 03:12:00 | Mercury | 0.0714 AU | 27.8 LD | 33.8 km/s |
| 2189-10-10 15:01:00 | Merc | 0.0563 AU | 21.9 LD | 36.4 km/s |
| 2189-10-10 15:01:00 | Mercury | 0.0563 AU | 21.9 LD | 36.4 km/s |
| 2195-04-23 22:27:00 | Merc | 0.0812 AU | 31.6 LD | 40.1 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB