2002 VC95 is a trans-Neptunian object in the Trans-Neptunian object orbit class. Its orbit takes it from 46.84 AU to 46.86 AU from the Sun; one orbit takes 320.7 years. Orbit from the JPL solution of 14 April 2021.
Where is it now
- Distance from Sun
- 46.856 AU
- True anomaly
- 226.37°
- Distance from Earth
- 46.274 AU
- As of
- 24 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
- 05h 42m 47s
- Declination
- +20° 53′ 17″
- Constellation
- Taurus
- Distance from Earth
- 46.26 AU
- Elongation from the Sun
- 126.11° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
From your location
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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
- 46.849 AU
- Eccentricity
- 0.0002
- Inclination
- 2.46°
- Orbital period
- 320.7 years
- Perihelion
- 46.838 AU
- Aphelion
- 46.859 AU
- Longitude of ascending node
- 176.76°
- Argument of periapsis
- 41.85°
- Epoch · J2000
- 2452600.5
- Orbit class · TNO
- Trans-Neptunian object
- Earth MOID · 17,835.0 LD
- 45.8281 AU
- Tisserand (Jupiter)
- 6.107
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 9).
- Observations used
- 11
- Data arc
- 18 days
- First observed
- 12 November 2002
- Last observed
- 30 November 2002
- Residual RMS
- 0.09 ″
- Solution · Otto Matic
- 14 April 2021
Visual & observation
- Absolute magnitude (H)
- 7.95
Discovery & classification
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB