Where is it now
- Distance from Sun
- 0.895 AU
- True anomaly
- 158.05°
- Distance from Earth
- 1.545 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
- 11h 18m 12s
- Declination
- +00° 55′ 41″
- Constellation
- Leo
- Distance from Earth
- 1.55 AU
- Elongation from the Sun
- 33.2° — 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
- 0.676 AU
- Eccentricity
- 0.382
- Inclination
- 9.82°
- Orbital period
- 203.2 days
- Perihelion
- 0.418 AU
- Aphelion
- 0.935 AU
- Longitude of ascending node
- 277.54°
- Argument of periapsis
- 56.65°
- Epoch · J2000
- 2461200.5
- Orbit class · IEO
- Atira (interior-Earth object)
- Earth MOID · 49.7 LD
- 0.1278 AU
- Tisserand (Jupiter)
- 8.349
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 26
- Data arc
- 7.83 years
- First observed
- 5 March 2016
- Last observed
- 3 January 2024
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 5 January 2024
Visual & observation
- Absolute magnitude (H)
- 20.11
Discovery & classification
Close approaches 285 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-11-22 18:14 UTC close approach of 2021 LJ4. Catalogue miss distance 168.1 LD · 6.46 × 10⁷ km. The curve is the geocentric path from 2028-11-19 to 2028-11-25, 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 |
|---|---|---|---|---|
| 2028-03-14 23:04:00 | Merc | 0.0523 AU | 20.4 LD | 14.8 km/s |
| 2028-03-14 23:04:00 | Mercury | 0.0523 AU | 20.4 LD | 14.8 km/s |
| 2028-11-22 18:14:00 | Earth | 0.432 AU | 168.1 LD | 9.8 km/s |
| 2029-02-26 06:35:00 | Earth | 0.3894 AU | 151.5 LD | 17.6 km/s |
| 2030-02-09 01:16:00 | Earth | 0.2625 AU | 102.1 LD | 14.8 km/s |
| 2030-05-04 16:18:00 | Earth | 0.3796 AU | 147.7 LD | 5.7 km/s |
| 2033-11-29 05:56:00 | Earth | 0.4115 AU | 160.1 LD | 8.5 km/s |
| 2034-02-27 13:23:00 | Earth | 0.3564 AU | 138.7 LD | 16.2 km/s |
| 2035-02-10 18:10:00 | Earth | 0.2962 AU | 115.3 LD | 16 km/s |
| 2035-05-13 02:54:00 | Earth | 0.4002 AU | 155.7 LD | 7.7 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