
Classical Kuiper belt object
Kuiper belt object, not controlled by an orbital resonance with Neptune

Kuiper belt object, not controlled by an orbital resonance with Neptune
A classical Kuiper belt object, also called a cubewano ( "QB1-o"), is a low-eccentricity Kuiper belt object (KBO) that orbits beyond Neptune and is not controlled by an orbital resonance with Neptune. Cubewanos have orbits with semi-major axes in the 40–50 AU range and, unlike Pluto, do not cross Neptune's orbit. That is, they have low-eccentricity and sometimes low-inclination orbits like the classical planets. The name "cubewano" derives from the first trans-Neptunian object (TNO) found after Pluto and Charon: 15760 Albion, which until January 2018 had only the provisional designation (15760) 1992 QB1. Similar objects found later were often called "QB1-os", or "cubewanos", after this object, though the term "classical" is much more frequently used in the scientific literature. Objects identified as cubewanos include: 15760 Albion (aka 1992 QB1 and gave rise to the term "Cubewano") Makemake, a dwarf planet Quaoar and 20000 Varuna, each considered the largest TNO at the time of discovery...
Read on Wikipedia · Image NASA/JHUAPL/SwRI/Roman Tkachenko, Public domain
Open boosters, collect cards and trade them. Free to play.
Play for free