Where is it now
- Distance from Sun
- 3.815 AU
- True anomaly
- 185.8°
- Distance from Earth
- 4.669 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 25m 09s
- Declination
- +03° 13′ 22″
- Constellation
- Leo
- Distance from Earth
- 4.66 AU
- Elongation from the Sun
- 28.32° — 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
- 2.427 AU
- Eccentricity
- 0.9807
- Inclination
- 19.74°
- Orbital period
- 3.78 years
- Perihelion
- 0.047 AU
- Aphelion
- 4.806 AU
- Longitude of ascending node
- 165.27°
- Argument of periapsis
- 172.41°
- Epoch · J2000
- 2453458.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 33.5 LD
- 0.086 AU
- Tisserand (Jupiter)
- 2.396
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 91
- Data arc
- 15.16 years
- First observed
- 1 May 1997
- Last observed
- 30 June 2012
- Residual RMS
- 0.11 ″
- Solution · Otto Matic
- 15 April 2021
Discovery & classification
Also known as 321P · 321P/1997 J6 · 321P/2001 D1 · 321P/2004 X7 · 321P/2008 S2 · 321P/2012 M2
Close approaches 30 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-04-01 04:36 UTC close approach of SOHO. Catalogue miss distance 124.3 LD · 4.78 × 10⁷ km. The curve is the geocentric path from 2031-03-29 to 2031-04-04, 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 |
|---|---|---|---|---|
| 2031-04-01 04:36:00 | Earth | 0.3194 AU | 124.3 LD | 34.4 km/s |
| 2035-01-28 07:12:00 | Venus | 0.0746 AU | 29.0 LD | 47.3 km/s |
| 2035-02-09 11:34:00 | Merc | 0.0466 AU | 18.1 LD | 75.1 km/s |
| 2035-02-09 11:34:00 | Mercury | 0.0466 AU | 18.1 LD | 75.1 km/s |
| 2039-11-20 09:36:00 | Juptr | 1.7972 AU | 699.4 LD | 14.8 km/s |
| 2050-03-11 02:14:00 | Earth | 0.2307 AU | 89.8 LD | 49.4 km/s |
| 2051-07-11 19:17:00 | Juptr | 1.1308 AU | 440.1 LD | 12.3 km/s |
| 2063-04-21 07:50:00 | Juptr | 0.7522 AU | 292.7 LD | 11 km/s |
| 2075-02-24 20:37:00 | Juptr | 0.6286 AU | 244.6 LD | 10.8 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- orbital elements: JPL SBDB