2017 FV241 is a trans-Neptunian object in the Trans-Neptunian object orbit class. Its orbit takes it from 31.41 AU to 64.23 AU from the Sun; one orbit takes 330.7 years. Orbit from the JPL solution of 29 August 2024.
Where is it now
- Distance from Sun
- 37.595 AU
- True anomaly
- 290.83°
- Distance from Earth
- 38.304 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
- 11h 06m 18s
- Declination
- -03° 18′ 41″
- Constellation
- Leo
- Distance from Earth
- 38.29 AU
- Elongation from the Sun
- 44.75° — near the Sun — look low at dusk or dawn
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
- 47.82 AU
- Eccentricity
- 0.3433
- Inclination
- 8.51°
- Orbital period
- 330.7 years
- Perihelion
- 31.405 AU
- Aphelion
- 64.234 AU
- Longitude of ascending node
- 255.73°
- Argument of periapsis
- 341.29°
- Epoch · J2000
- 2461200.5
- Orbit class · TNO
- Trans-Neptunian object
- Earth MOID · 11,828.9 LD
- 30.3949 AU
- Tisserand (Jupiter)
- 5.741
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 25
- Data arc
- 4.21 years
- First observed
- 17 January 2015
- Last observed
- 5 April 2019
- Residual RMS
- 0.17 ″
- Solution · Otto Matic
- 29 August 2024
Visual & observation
- Absolute magnitude (H)
- 9.16
Discovery & classification
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB