2012 VB116 is a trans-Neptunian object in the Trans-Neptunian object orbit class. Its orbit takes it from 39.77 AU to 55.04 AU from the Sun; one orbit takes 326.4 years. Orbit from the JPL solution of 5 June 2026.
Where is it now
- Distance from Sun
- 46.678 AU
- True anomaly
- 266.16°
- Distance from Earth
- 46.278 AU
- As of
- 25 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
- 06h 25m 40s
- Declination
- +00° 02′ 14″
- Constellation
- Monoceros
- Distance from Earth
- 46.28 AU
- Elongation from the Sun
- 113.23° — well clear of the Sun
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
- 47.404 AU
- Eccentricity
- 0.161
- Inclination
- 23.22°
- Orbital period
- 326.4 years
- Perihelion
- 39.772 AU
- Aphelion
- 55.035 AU
- Longitude of ascending node
- 193.54°
- Argument of periapsis
- 356.71°
- Epoch · J2000
- 2461200.5
- Orbit class · TNO
- Trans-Neptunian object
- Earth MOID · 15,089.5 LD
- 38.7733 AU
- Tisserand (Jupiter)
- 5.585
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 131
- Data arc
- 15 years
- First observed
- 12 January 2011
- Last observed
- 11 January 2026
- Residual RMS
- 0.49 ″
- Solution · Otto Matic
- 5 June 2026
Visual & observation
- Absolute magnitude (H)
- 5.17
Discovery & classification
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB