Where is it now
- Distance from Sun
- 6.167 AU
- True anomaly
- 193.09°
- Distance from Earth
- 7.158 AU
- As of
- 22 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
- 13h 40m 24s
- Declination
- -06° 54′ 57″
- Constellation
- Virgo
- Distance from Earth
- 7.16 AU
- Elongation from the Sun
- 5.17° — too close to the Sun to observe
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
- 3.839 AU
- Eccentricity
- 0.7073
- Inclination
- 16.98°
- Orbital period
- 7.52 years
- Perihelion
- 1.124 AU
- Aphelion
- 6.554 AU
- Longitude of ascending node
- 37.68°
- Argument of periapsis
- 333.8°
- Epoch · J2000
- 2456908.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 60.8 LD
- 0.1564 AU
- Tisserand (Jupiter)
- 2.517
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 88
- Data arc
- 22.59 years
- First observed
- 11 November 1991
- Last observed
- 15 June 2014
- Residual RMS
- 1.11 ″
- Solution · Ryan S. Park
- 29 August 2014
Visual & observation
- Absolute magnitude (H)
- 16.3
- Total magnitude M₁ · K₁ 17
- 16.3
Discovery & classification
Also known as 181P · 181P/1991 V1 · 181P/1991b1 · 181P/2006 U4 · 1991 XVIII
Close approaches 13 on record
Top-down view of the ecliptic, Earth at the centre, for the 2067-10-06 00:38 UTC close approach of Shoemaker-Levy. Catalogue miss distance 169.6 LD · 6.52 × 10⁷ km. The curve is the geocentric path from 2067-10-03 to 2067-10-09, 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. The path is approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2040-07-13 11:12:00 | Juptr | 1.2752 AU | 496.3 LD | 6.7 km/s |
| 2065-02-14 11:07:00 | Juptr | 0.7612 AU | 296.2 LD | 6.9 km/s |
| 2067-10-06 00:38:00 | Earth | 0.4357 AU | 169.6 LD | 11.7 km/s |
| 2088-12-22 22:55:00 | Juptr | 0.1673 AU | 65.1 LD | 8.4 km/s |
| 2088-12-22 22:55:00 | Jupiter | 0.1673 AU | 65.1 LD | 8.4 km/s |
| 2111-01-02 23:53:00 | Juptr | 1.4155 AU | 550.9 LD | 6.4 km/s |
| 2141-10-01 14:05:00 | Earth | 0.379 AU | 147.5 LD | 8.4 km/s |
| 2148-03-22 17:22:00 | Jupiter | 0.1597 AU | 62.1 LD | 8.6 km/s |
| 2148-03-22 17:22:00 | Juptr | 0.1597 AU | 62.1 LD | 8.6 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)
- visual properties: JPL SBDB (lookup)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB