Where is it now
- Distance from Sun
- 2.024 AU
- True anomaly
- 253.01°
- Distance from Earth
- 1.083 AU
- As of
- 11 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
- 02h 04m 24s
- Declination
- -15° 51′ 23″
- Constellation
- Cetus
- Distance from Earth
- 1.08 AU
- Elongation from the Sun
- 153.12° — 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
- 2.931 AU
- Eccentricity
- 0.6663
- Inclination
- 16.91°
- Orbital period
- 5.02 years
- Perihelion
- 0.978 AU
- Aphelion
- 4.884 AU
- Longitude of ascending node
- 75.1°
- Argument of periapsis
- 51.44°
- Epoch · J2000
- 2453294.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 42.4 LD
- 0.1088 AU
- Tisserand (Jupiter)
- 2.846
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 200
- Data arc
- 15.01 years
- First observed
- 26 October 2001
- Last observed
- 29 October 2016
- Residual RMS
- 0.68 ″
- Solution · Otto Matic
- 31 October 2024
Visual & observation
- Absolute magnitude (H)
- 20.8
- Total magnitude M₁ · K₁ 4.5
- 20.8
Discovery & classification
Also known as 182P · 182P/2001 WF2 · 182P/2006 W2
Close approaches 23 on record
Top-down view of the ecliptic, Earth at the centre, for the 2057-12-07 20:26 UTC close approach of LONEOS. Catalogue miss distance 124.4 LD · 4.78 × 10⁷ km. The curve is the geocentric path from 2057-12-04 to 2057-12-10, 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 |
|---|---|---|---|---|
| 2044-04-27 00:34:00 | Juptr | 1.0964 AU | 426.7 LD | 8 km/s |
| 2057-12-07 20:26:00 | Earth | 0.3197 AU | 124.4 LD | 19.9 km/s |
| 2063-03-14 02:27:00 | Earth | 0.3711 AU | 144.4 LD | 16 km/s |
| 2079-12-29 11:26:00 | Juptr | 1.4238 AU | 554.1 LD | 9.7 km/s |
| 2092-06-19 18:37:00 | Juptr | 1.7608 AU | 685.3 LD | 9.5 km/s |
| 2099-01-02 19:27:00 | Earth | 0.1914 AU | 74.5 LD | 10.3 km/s |
| 2128-02-26 06:40:00 | Juptr | 1.2917 AU | 502.7 LD | 7.1 km/s |
| 2139-12-24 08:06:00 | Earth | 0.1533 AU | 59.7 LD | 12.5 km/s |
| 2145-03-25 19:59:00 | Earth | 0.3918 AU | 152.5 LD | 19 km/s |
| 2163-09-21 08:33:00 | Juptr | 1.2252 AU | 476.8 LD | 6.6 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB