- 000 AU,
beyond the
aphelia of the
three known sednoids. One
attempt at a
precise definition of
sednoids is any body with a
perihelion greater than 50 AU...
-
perihelion orbits similar to that of
Sedna are
termed sednoids. As of 2024,
there are
three known sednoids: Sedna, 2012 VP113, and Leleākūhonua.
These objects...
-
strongly influenced by it.
Among the
extreme trans-Neptunian
objects are the
sednoids, four
objects with an
outstandingly high perihelion: Sedna, 2012 VP113...
-
objects of the
Kuiper belt, the
scattered disc and
detached objects with the
sednoids being the most
distant ones. As of
February 2025, the
catalog of minor...
- the
prototype of a new
orbit class of
objects named after itself, the
sednoids,
which include 2012 VP113 and Leleākūhonua, both
celestial bodies with...
- and the
extreme trans-Neptunian
objects including the ESDOs, EDDOs, and
sednoids,
which have a semi-major axis of at
least 150 AU and a
perihelion (closest...
- (1:2 resonance)
Scattered disc
objects (SDOs)
Resonant SDOs
Extreme trans-Neptunian
object Detached objects Sednoids Oort
cloud objects (ICO/OCOs) v t e...
- the centaurs, the
Kuiper belt objects, the
scattered disc objects, the
sednoids, and the Oort
cloud objects.
About 60% of the main belt m**** is contained...
- than the
scattered ETNOs, but are
still relatively close to Neptune. The
sednoids or
inner Oort
cloud objects, with
perihelia beyond 50–60 AU, are too far...
- (provisional
designation 2015 TG387) is an
extreme trans-Neptunian
object and
sednoid in the
outermost part of the
Solar System. It was
first observed on 13...
