Where is it now
- Distance from Sun
- 2.808 AU
- True anomaly
- 236.23°
- Distance from Earth
- 3.694 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
- 11h 35m 51s
- Declination
- -13° 17′ 31″
- Constellation
- Crater
- Distance from Earth
- 3.69 AU
- Elongation from the Sun
- 23.96° — 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
- 2.918 AU
- Eccentricity
- 0.5976
- Inclination
- 20.4°
- Orbital period
- 4.98 years
- Perihelion
- 1.174 AU
- Aphelion
- 4.661 AU
- Longitude of ascending node
- 282.2°
- Argument of periapsis
- 15.31°
- Epoch · J2000
- 2454804.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 65.0 LD
- 0.167 AU
- Tisserand (Jupiter)
- 2.909
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 1,469
- Data arc
- 20.07 years
- First observed
- 30 July 2002
- Last observed
- 24 August 2022
- Residual RMS
- 0.75 ″
- Solution · Otto Matic
- 26 August 2022
Visual & observation
- Absolute magnitude (H)
- 19.1
- Total magnitude M₁ · K₁ 4.5
- 19.1
Discovery & classification
Also known as 189P · 189P/2002 O5 · 189P/2007 N2
Close approaches 26 on record
Top-down view of the ecliptic, Earth at the centre, for the 2073-06-30 14:14 UTC close approach of NEAT. Catalogue miss distance 189.7 LD · 7.29 × 10⁷ km. The curve is the geocentric path from 2073-06-27 to 2073-07-03, 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 |
|---|---|---|---|---|
| 2049-09-30 02:44:00 | Juptr | 0.8206 AU | 319.3 LD | 6.7 km/s |
| 2073-06-30 14:14:00 | Earth | 0.4874 AU | 189.7 LD | 16.3 km/s |
| 2078-07-16 07:08:00 | Earth | 0.434 AU | 168.9 LD | 12 km/s |
| 2085-06-29 12:22:00 | Juptr | 1.5063 AU | 586.2 LD | 8.5 km/s |
| 2097-04-15 10:40:00 | Juptr | 1.8976 AU | 738.5 LD | 8.8 km/s |
| 2109-07-16 03:17:00 | Earth | 0.3854 AU | 150.0 LD | 11.4 km/s |
| 2132-11-10 14:48:00 | Juptr | 1.0162 AU | 395.5 LD | 6.1 km/s |
| 2145-06-26 15:58:00 | Earth | 0.3913 AU | 152.3 LD | 16.5 km/s |
| 2150-07-10 19:32:00 | Earth | 0.1811 AU | 70.5 LD | 11.6 km/s |
| 2155-07-26 13:42:00 | Earth | 0.4578 AU | 178.2 LD | 13.4 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