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2018 VM35

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2018 VM35
Designations
2018 VM35
TNO
Orbital characteristics [2]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 7
Observation arc89 days
Aphelion426.59 AU
Perihelion45.348 AU
235.97 AU
Eccentricity0.8078
3624.80 yr (1,323,959 d)
356.17°
0° 0m 1.08s / day
Inclination8.4875°
192.53°
301.94°
Physical characteristics
7.7236[2]

2018 VM35, is a trans-Neptunian object from the outermost region of the Solar System. With a perihelion distance greater than 40 AU, it is considered a detached object.

Orbit and classification

2018 VM35 orbits the Sun at a distance of 45.3–426.6 AU once every 3624 years and 10 months (1,323,959 days; semi-major axis of 235.97 AU). Its orbit has an eccentricity of 0.81 and an inclination of 8° with respect to the ecliptic.[2]

References

  1. ^ "2018 VM35". Minor Planet Center. Retrieved 22 February 2019.
  2. ^ a b c "JPL Small-Body Database Browser: (2018 VM35)" (2019-02-03 last obs.). Jet Propulsion Laboratory. Retrieved 22 February 2019.
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