Kuiper belt
The Kuiper belt is an area of the Solar System beyond the orbit of Neptune (at 30 astronomical units) to 50 AU from the Sun.
The objects within the Kuiper Belt together with the members of the scattered disk beyond, are together called trans-Neptunian.
Many objects such as dwarf planets in the Kuiper belt are much bigger than the ones in the asteroid belt and are round. At least some Kuiper belt objects are icebound.
The first objects in the Kuiper belt to be found were Pluto and Charon (moon) but the belt was only identified and named in 1992 when more Kuiper belt objects (KBOs) were found. A few thousand have since been discovered and more than 70,000 KBOs over 100 km (62 mi) in diameter are thought to exist.
Kuiper Belt Media
Charon and Pluto: Strikingly Different Worlds*A composite of enhanced color images of Pluto (lower right) and Charon (upper left), taken by NASA's New Horizons spacecraft as it passed through the Pluto system on July 14, 2015. This image highlights the striking differences between Pluto and Charon. The color and bright
Astronomer Gerard Kuiper, after whom the Kuiper belt is named
In 1980, astronomer Julio Fernandez predicted the existence of a belt. It has been said that because the words "Kuiper" and "comet belt" appeared in the opening sentence of Fernandez's paper, this hypothetical region was referred to as the "Kuiper belt".
The array of telescopes atop Mauna Kea, with which the Kuiper belt was discovered
Distribution of cubewanos (blue), Resonant trans-Neptunian objects (red), Sednoids (yellow) and scattered objects (grey)
Orbit classification (schematic of semi-major axes)