Where is it now
- Distance from Sun
- 4.358 AU
- True anomaly
- 203.18°
- Distance from Earth
- 3.605 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
- 22h 39m 57s
- Declination
- -21° 09′ 25″
- Constellation
- Aquarius
- Distance from Earth
- 3.61 AU
- Elongation from the Sun
- 133.27° — 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
- 3.06 AU
- Eccentricity
- 0.5878
- Inclination
- 11.54°
- Orbital period
- 5.35 years
- Perihelion
- 1.261 AU
- Aphelion
- 4.859 AU
- Longitude of ascending node
- 105.81°
- Argument of periapsis
- 34.57°
- Epoch · J2000
- 2458413.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 116.4 LD
- 0.299 AU
- Tisserand (Jupiter)
- 2.916
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 771
- Data arc
- 16.66 years
- First observed
- 10 November 2006
- Last observed
- 8 July 2023
- Residual RMS
- 0.53 ″
- Solution · Otto Matic
- 6 June 2024
Visual & observation
- Absolute magnitude (H)
- 18.6
- Total magnitude M₁ · K₁ 4.5
- 18.6
Discovery & classification
Also known as 263P · 263P/2006 Y2 · 263P/2012 K9
Close approaches 18 on record
Top-down view of the ecliptic, Earth at the centre, for the 2087-02-01 22:25 UTC close approach of Gibbs. Catalogue miss distance 125.6 LD · 4.83 × 10⁷ km. The curve is the geocentric path from 2087-01-29 to 2087-02-04, 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 |
|---|---|---|---|---|
| 2056-09-15 22:34:00 | Juptr | 0.9215 AU | 358.6 LD | 7.8 km/s |
| 2069-03-30 10:46:00 | Juptr | 0.8624 AU | 335.6 LD | 6.3 km/s |
| 2087-02-01 22:25:00 | Earth | 0.3227 AU | 125.6 LD | 8.4 km/s |
| 2116-06-23 20:17:00 | Juptr | 0.6067 AU | 236.1 LD | 5.2 km/s |
| 2124-02-09 05:49:00 | Earth | 0.3521 AU | 137.0 LD | 6.2 km/s |
| 2151-10-25 10:06:00 | Juptr | 1.8167 AU | 707.0 LD | 10.9 km/s |
| 2164-03-10 14:16:00 | Juptr | 0.8147 AU | 317.0 LD | 6.4 km/s |
| 2166-01-14 08:43:00 | Earth | 0.4262 AU | 165.9 LD | 15.2 km/s |
| 2199-06-22 15:19:00 | Juptr | 0.616 AU | 239.7 LD | 5.3 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