Where is it now
- Distance from Sun
- 5.004 AU
- True anomaly
- 182.83°
- Distance from Earth
- 4.326 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 13m 38s
- Declination
- -22° 21′ 56″
- Constellation
- Aquarius
- Distance from Earth
- 4.33 AU
- Elongation from the Sun
- 127.39° — 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
- 3.186 AU
- Eccentricity
- 0.5733
- Inclination
- 9.84°
- Orbital period
- 5.69 years
- Perihelion
- 1.359 AU
- Aphelion
- 5.012 AU
- Longitude of ascending node
- 87.44°
- Argument of periapsis
- 66.4°
- Epoch · J2000
- 2458101.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 159.9 LD
- 0.411 AU
- Tisserand (Jupiter)
- 2.897
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 403
- Data arc
- 6.52 years
- First observed
- 24 November 2011
- Last observed
- 2 June 2018
- Residual RMS
- 0.48 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 17
- Total magnitude M₁ · K₁ 11
- 17
Discovery & classification
Also known as 365P · 365P/2011 WG113 · 365P/2017 U6
Close approaches 15 on record
Top-down view of the ecliptic, Earth at the centre, for the 2046-02-27 21:55 UTC close approach of PANSTARRS. Catalogue miss distance 161.3 LD · 6.2 × 10⁷ km. The curve is the geocentric path from 2046-02-24 to 2046-03-02, 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 |
|---|---|---|---|---|
| 2046-02-27 21:55:00 | Earth | 0.4146 AU | 161.3 LD | 3.8 km/s |
| 2085-02-25 07:26:00 | Earth | 0.4045 AU | 157.4 LD | 3.3 km/s |
| 2092-07-31 04:05:00 | Juptr | 0.9937 AU | 386.7 LD | 7.9 km/s |
| 2102-02-09 21:41:00 | Mars | 0.0833 AU | 32.4 LD | 11.1 km/s |
| 2104-06-14 05:01:00 | Juptr | 0.6541 AU | 254.6 LD | 6 km/s |
| 2116-04-07 04:53:00 | Juptr | 0.7629 AU | 296.9 LD | 6.7 km/s |
| 2128-04-21 15:09:00 | Juptr | 1.9304 AU | 751.3 LD | 11 km/s |
| 2200-06-18 09:15:00 | Juptr | 1.0924 AU | 425.1 LD | 8.3 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)
- visual properties: JPL SBDB (lookup)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB