2005 LX36
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2005 LX36 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.44 AU to 1.62 AU from the Sun; one orbit takes 381.8 days. Orbit from the JPL solution of 11 June 2026.
Where is it now
- Distance from Sun
- 1.529 AU
- True anomaly
- 197.3°
- Distance from Earth
- 1.625 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 50m 02s
- Declination
- +06° 56′ 09″
- Constellation
- Aquila
- Distance from Earth
- 1.63 AU
- Elongation from the Sun
- 66.13° — well clear of the Sun
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
- 1.03 AU
- Eccentricity
- 0.5754
- Inclination
- 32.97°
- Orbital period
- 381.8 days
- Perihelion
- 0.437 AU
- Aphelion
- 1.623 AU
- Longitude of ascending node
- 252.73°
- Argument of periapsis
- 239.13°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 8.9 LD
- 0.0229 AU
- Tisserand (Jupiter)
- 5.663
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 73
- Data arc
- 20.99 years
- First observed
- 14 June 2005
- Last observed
- 11 June 2026
- Residual RMS
- 0.65 ″
- Solution · Otto Matic
- 11 June 2026
Visual & observation
- Absolute magnitude (H)
- 20.93
Discovery & classification
Close approaches 18 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-06-03 01:02 UTC close approach of 2005 LX36. Catalogue miss distance 21.8 LD · 8.38 × 10⁶ km. The curve is the geocentric path from 2028-05-31 to 2028-06-06, 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 |
|---|---|---|---|---|
| 2028-06-03 01:02:00 | Earth | 0.056 AU | 21.8 LD | 22.3 km/s |
| 2051-06-01 11:28:00 | Earth | 0.132 AU | 51.4 LD | 20.6 km/s |
| 2052-06-09 20:21:00 | Earth | 0.1298 AU | 50.5 LD | 26.5 km/s |
| 2075-06-07 20:55:00 | Earth | 0.0623 AU | 24.2 LD | 24.8 km/s |
| 2098-06-06 03:03:00 | Earth | 0.0297 AU | 11.6 LD | 23.8 km/s |
| 2121-06-07 01:12:00 | Earth | 0.0316 AU | 12.3 LD | 23.9 km/s |
| 2143-06-01 03:05:00 | Earth | 0.1978 AU | 77.0 LD | 19.4 km/s |
| 2144-06-08 18:32:00 | Earth | 0.0728 AU | 28.3 LD | 25.1 km/s |
| 2166-06-02 15:33:00 | Earth | 0.1284 AU | 50.0 LD | 20.7 km/s |
| 2167-06-12 10:48:00 | Earth | 0.1408 AU | 54.8 LD | 26.8 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