- A
classical Kuiper belt object, also
called a
cubewano (/ˌkjuːbiːˈwʌnoʊ/ "QB1-o"), is a low-eccentricity
Kuiper belt
object (KBO) that
orbits beyond Neptune...
-
types of TNO subgroups:
classical Kuiper belt objects, also
known as "
cubewanos", the
resonant trans-Neptunian
objects with
their main and higher-order...
-
resonance with Neptune, and the
classical Kuiper belt objects, also
called "
cubewanos", that have no such resonance,
moving on
almost circular orbits, unperturbed...
- ≈ 2.018 0.51 (naming rules)
resonant cubewano 136472
Makemake 1430+38 −22 1.9±0.2 0.81 (naming rules) hot
cubewano 225088
Gonggong 1230±50 1.74±0.16 0...
- It is a "cold"
classical Kuiper belt
object and gave rise to the name
cubewano for this kind of object,
after the QB1
portion of its designation. Decoding...
- to 47.7 AU.
Members of the
classical Kuiper belt are
sometimes called "
cubewanos",
after the
first of
their kind to be discovered,
originally designated...
-
Kuiper belt in the
outermost region of the
Solar System, also
known as a
cubewano. With a
likely diameter of at
least 600
kilometers (400 miles), it is approximately...
-
Solar System,
approximately 340
kilometers (210 miles) in diameter. The
cubewano belongs to the hot po****tion. It was
discovered on 26 July 2011, by astronomers...
- 19521
Chaos is a
cubewano, a Kuiper-belt
object not in
resonance with any planet.
Chaos was
discovered in 1998 by the Deep
Ecliptic Survey with Kitt Peak's...
- M 2002 MS4 307261 398±12 – –
cubewano 2002 AW197 55565 384±19 – –
cubewano Varda 174567 373±8 245±6 1.23±0.04
cubewano;
binary · 2013 FY27 532037 370±40...
