Where is it now
- Distance from Sun
- 1.137 AU
- True anomaly
- 207.4°
- Distance from Earth
- 1.938 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
- 15h 32m 09s
- Declination
- -18° 07′ 44″
- Constellation
- Libra
- Distance from Earth
- 1.94 AU
- Elongation from the Sun
- 26.4° — near the Sun — look low at dusk or dawn
Favours the southern hemisphere; low or below the horizon from far north.
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
- 0.917 AU
- Eccentricity
- 0.2987
- Inclination
- 1.66°
- Orbital period
- 320.9 days
- Perihelion
- 0.643 AU
- Aphelion
- 1.191 AU
- Longitude of ascending node
- 180.17°
- Argument of periapsis
- 230.21°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.5 LD
- 0.0038 AU
- Tisserand (Jupiter)
- 6.473
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 156
- Data arc
- 469 days
- First observed
- 15 March 2021
- Last observed
- 27 June 2022
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 29 June 2022
Physical properties
- Rotation period
- 0.14 hours
Visual & observation
- Absolute magnitude (H)
- 25.78
Discovery & classification
Close approaches 203 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-03-17 07:42 UTC close approach of 2021 EL4. Catalogue miss distance 68.2 LD · 2.62 × 10⁷ km. The curve is the geocentric path from 2028-03-14 to 2028-03-20, 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 |
|---|---|---|---|---|
| 2028-03-17 07:42:00 | Earth | 0.1753 AU | 68.2 LD | 13.6 km/s |
| 2028-11-28 02:50:00 | Earth | 0.3386 AU | 131.8 LD | 11.8 km/s |
| 2029-06-22 22:25:00 | Earth | 0.1158 AU | 45.1 LD | 5.8 km/s |
| 2032-06-21 17:11:00 | Venus | 0.0405 AU | 15.7 LD | 8.6 km/s |
| 2035-03-26 01:56:00 | Earth | 0.3734 AU | 145.3 LD | 19.7 km/s |
| 2035-12-28 07:23:00 | Earth | 0.2962 AU | 115.3 LD | 9.3 km/s |
| 2036-05-12 03:24:00 | Earth | 0.1837 AU | 71.5 LD | 6.6 km/s |
| 2036-09-13 21:01:00 | Earth | 0.2855 AU | 111.1 LD | 8.3 km/s |
| 2037-06-23 01:19:00 | Earth | 0.3947 AU | 153.6 LD | 20.2 km/s |
| 2038-08-19 13:11:00 | Venus | 0.0458 AU | 17.8 LD | 9.7 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