Where is it now
- Distance from Sun
- 0.856 AU
- True anomaly
- 60.4°
- Distance from Earth
- 0.663 AU
- As of
- 21 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 09m 43s
- Declination
- +10° 53′ 56″
- Constellation
- Leo
- Distance from Earth
- 0.66 AU
- Elongation from the Sun
- 58.16° — 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
- 0.913 AU
- Eccentricity
- 0.1084
- Inclination
- 0.63°
- Orbital period
- 318.6 days
- Perihelion
- 0.814 AU
- Aphelion
- 1.012 AU
- Longitude of ascending node
- 219.1°
- Argument of periapsis
- 149.96°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.7 LD
- 0.0019 AU
- Tisserand (Jupiter)
- 6.532
Orbit quality
Orbit reasonably well determined (uncertainty code 4).
- Observations used
- 154
- Data arc
- 37 days
- First observed
- 10 March 2026
- Last observed
- 16 April 2026
- Residual RMS
- 0.33 ″
- Solution · Otto Matic
- 29 May 2026
Visual & observation
- Absolute magnitude (H)
- 26.15
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 36 on record
Top-down view of the ecliptic, Earth at the centre, for the 2032-11-27 03:15 UTC close approach of 2026 EL2. Catalogue miss distance 55.7 LD · 2.14 × 10⁷ km. The curve is the geocentric path from 2032-11-24 to 2032-11-30, 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 |
|---|---|---|---|---|
| 2032-11-27 03:15:00 | Earth | 0.1431 AU | 55.7 LD | 3.3 km/s |
| 2033-04-30 00:07:00 | Earth | 0.0874 AU | 34.0 LD | 5 km/s |
| 2035-05-03 07:09:00 | Venus | 0.1166 AU | 45.4 LD | 0.6 km/s |
| 2039-10-06 03:01:00 | Earth | 0.1877 AU | 73.0 LD | 5 km/s |
| 2045-11-02 14:32:00 | Venus | 0.1001 AU | 39.0 LD | 1.1 km/s |
| 2046-08-18 11:54:00 | Earth | 0.1779 AU | 69.2 LD | 4.5 km/s |
| 2053-02-15 17:14:00 | Earth | 0.0233 AU | 9.1 LD | 2.9 km/s |
| 2053-06-19 14:55:00 | Earth | 0.1095 AU | 42.6 LD | 1.5 km/s |
| 2060-02-15 23:28:00 | Earth | 0.1935 AU | 75.3 LD | 8.3 km/s |
| 2060-08-20 01:20:00 | Earth | 0.1702 AU | 66.2 LD | 4.3 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