2022 LE1 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.62 AU to 1.41 AU from the Sun; one orbit takes 371.9 days. Orbit from the JPL solution of 6 June 2022.
Where is it now
- Distance from Sun
- 1.405 AU
- True anomaly
- 184.76°
- Distance from Earth
- 1.571 AU
- As of
- 3 November 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
- 18h 58m 13s
- Declination
- -41° 50′ 12″
- Constellation
- Corona Australis
- Distance from Earth
- 1.57 AU
- Elongation from the Sun
- 61.6° — well clear of the Sun
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
- 1.012 AU
- Eccentricity
- 0.3915
- Inclination
- 23.11°
- Orbital period
- 371.9 days
- Perihelion
- 0.616 AU
- Aphelion
- 1.408 AU
- Longitude of ascending node
- 76.04°
- Argument of periapsis
- 63.12°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 7.0 LD
- 0.018 AU
- Tisserand (Jupiter)
- 5.888
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 68
- Data arc
- 24 hours
- First observed
- 5 June 2022
- Last observed
- 6 June 2022
- Residual RMS
- 0.32 ″
- Solution · Otto Matic
- 6 June 2022
Visual & observation
- Absolute magnitude (H)
- 25.82
Discovery & classification
Close approaches 72 on record
Top-down view of the ecliptic, Earth at the centre, for the 2060-10-15 01:59 UTC close approach of 2022 LE1. Catalogue miss distance 191.4 LD · 7.36 × 10⁷ km. The curve is the geocentric path from 2060-10-12 to 2060-10-18, 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 |
|---|---|---|---|---|
| 2049-08-22 15:23:00 | Venus | 0.0897 AU | 34.9 LD | 20 km/s |
| 2060-10-15 01:59:00 | Earth | 0.4919 AU | 191.4 LD | 27.4 km/s |
| 2061-10-22 01:41:00 | Earth | 0.3991 AU | 155.3 LD | 24.5 km/s |
| 2062-10-29 13:36:00 | Earth | 0.3138 AU | 122.1 LD | 21.9 km/s |
| 2063-11-06 19:43:00 | Earth | 0.245 AU | 95.4 LD | 19.5 km/s |
| 2064-11-15 05:23:00 | Earth | 0.2089 AU | 81.3 LD | 17.7 km/s |
| 2065-11-26 02:25:00 | Earth | 0.2185 AU | 85.0 LD | 16.5 km/s |
| 2066-12-08 15:24:00 | Earth | 0.2624 AU | 102.1 LD | 16.2 km/s |
| 2067-12-22 13:19:00 | Earth | 0.3195 AU | 124.3 LD | 16.5 km/s |
| 2069-01-05 03:57:00 | Earth | 0.3756 AU | 146.2 LD | 16.9 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