Where is it now
- Distance from Sun
- 7.603 AU
- True anomaly
- 195.05°
- Distance from Earth
- 8.165 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
- 16h 38m 43s
- Declination
- -22° 26′ 16″
- Constellation
- Ophiuchus
- Distance from Earth
- 8.17 AU
- Elongation from the Sun
- 52.19° — near the Sun — look low at dusk or dawn
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
- 4.799 AU
- Eccentricity
- 0.736
- Inclination
- 8.9°
- Orbital period
- 10.51 years
- Perihelion
- 1.267 AU
- Aphelion
- 8.331 AU
- Longitude of ascending node
- 259.36°
- Argument of periapsis
- 162.78°
- Epoch · J2000
- 2457120.5
- Orbit class · JFc
- Jupiter-family comet (P < 20 y)
- Earth MOID · 111.1 LD
- 0.2855 AU
- Tisserand (Jupiter)
- 2.369
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 347
- Data arc
- 11.1 years
- First observed
- 22 December 2008
- Last observed
- 29 January 2020
- Residual RMS
- 0.74 ″
- Solution · Otto Matic
- 2 May 2021
Visual & observation
- Absolute magnitude (H)
- 14.2
- Total magnitude M₁ · K₁ 20
- 14.2
Discovery & classification
Also known as 387P · 387P/2008 Y1 · 387P/2019 R1
Close approaches 12 on record
Top-down view of the ecliptic, Earth at the centre, for the 2163-11-27 11:17 UTC close approach of Boattini. Catalogue miss distance 67.7 LD · 2.6 × 10⁷ km. The curve is the geocentric path from 2163-11-24 to 2163-11-30, 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 a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2053-02-10 05:37:00 | Juptr | 0.9097 AU | 354.0 LD | 8.8 km/s |
| 2091-01-27 03:35:00 | Juptr | 0.9053 AU | 352.3 LD | 11.9 km/s |
| 2124-09-11 01:29:00 | Juptr | 1.5277 AU | 594.6 LD | 13.2 km/s |
| 2162-05-08 02:54:00 | Jupiter | 0.4902 AU | 190.8 LD | 10.5 km/s |
| 2162-05-08 02:54:00 | Juptr | 0.4902 AU | 190.8 LD | 10.5 km/s |
| 2163-11-27 11:17:00 | Earth | 0.1739 AU | 67.7 LD | 8.1 km/s |
| 2195-08-14 21:43:00 | Juptr | 1.0403 AU | 404.9 LD | 8.1 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