2013 RS124 is a trans-Neptunian object in the Trans-Neptunian object orbit class. Its orbit takes it from 34.77 AU to 58.42 AU from the Sun; one orbit takes 318.1 years. Orbit from the JPL solution of 14 July 2022.
Where is it now
- Distance from Sun
- 34.772 AU
- True anomaly
- 0.37°
- Distance from Earth
- 33.823 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
- 02h 49m 07s
- Declination
- +00° 03′ 22″
- Constellation
- Cetus
- Distance from Earth
- 33.82 AU
- Elongation from the Sun
- 162.67° — near opposition — up most of the night
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
- 46.595 AU
- Eccentricity
- 0.2537
- Inclination
- 15.28°
- Orbital period
- 318.1 years
- Perihelion
- 34.772 AU
- Aphelion
- 58.418 AU
- Longitude of ascending node
- 140.09°
- Argument of periapsis
- 259.52°
- Epoch · J2000
- 2461200.5
- Orbit class · TNO
- Trans-Neptunian object
- Earth MOID · 13,159.2 LD
- 33.8134 AU
- Tisserand (Jupiter)
- 5.696
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 32
- Data arc
- 7.03 years
- First observed
- 10 September 2013
- Last observed
- 21 September 2020
- Residual RMS
- 0.16 ″
- Solution · Otto Matic
- 14 July 2022
Visual & observation
- Absolute magnitude (H)
- 8.1
Discovery & classification
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB