2015 VG169 is a trans-Neptunian object in the Trans-Neptunian object orbit class. Its orbit takes it from 44.08 AU to 49.61 AU from the Sun; one orbit takes 320.6 years. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 44.218 AU
- True anomaly
- 19.14°
- Distance from Earth
- 43.366 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
- 04h 03m 40s
- Declination
- +18° 41′ 24″
- Constellation
- Taurus
- Distance from Earth
- 43.36 AU
- Elongation from the Sun
- 149.54° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 46.846 AU
- Eccentricity
- 0.059
- Inclination
- 2.18°
- Orbital period
- 320.6 years
- Perihelion
- 44.082 AU
- Aphelion
- 49.611 AU
- Longitude of ascending node
- 127.35°
- Argument of periapsis
- 275.4°
- Epoch · J2000
- 2461200.5
- Orbit class · TNO
- Trans-Neptunian object
- Earth MOID · 16,769.7 LD
- 43.0906 AU
- Tisserand (Jupiter)
- 6.097
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 33
- Data arc
- 801 days
- First observed
- 17 November 2014
- Last observed
- 26 January 2017
- Residual RMS
- 0.16 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 8.1
Discovery & classification
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB