The Solar System Beyond The Planets

@inproceedings{Delsanti2006TheSS,
  title={The Solar System Beyond The Planets},
  author={Audrey C. Delsanti and David C. Jewitt},
  year={2006}
}
The Kuiper belt contains a vast number of objects in a flattened, ring-like volume beyond the orbit of Neptune. These objects are collisionally processed relics from the accretion disk of the Sun and, as such, they can reveal much about early conditions in the Solar system. At the cryogenic temperatures prevailing beyond Neptune, volatile ices have been able to survive since the formation epoch 4.5 Gyr ago. The Kuiper belt is the source of the Centaurs and the Jupiter-family comets. It is also… 
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AN OUTER PLANET BEYOND PLUTO AND THE ORIGIN OF THE TRANS-NEPTUNIAN BELT ARCHITECTURE
Trans-Neptunian objects (TNOs) are remnants of a collisionally and dynamically evolved planetesimal disk in the outer solar system. This complex structure, known as the trans-Neptunian belt (or
Mass of the Kuiper belt
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Origin and Evolution of the Cometary Reservoirs
Comets have three known reservoirs: the roughly spherical Oort Cloud (for long-period comets), the flattened Kuiper Belt (for ecliptic comets), and, surprisingly, the asteroid belt (for main-belt
Trans-Neptunian Objects as Natural Probes to the Unknown Solar System
Trans-Neptunian objects (TNOs) are icy/rocky bodies that move beyond the orbit of Neptune in a region known as the trans-Neptunian belt (or Edgeworth-Kuiper belt). In contrast to the predictions of
The Edgeworth-Kuiper debris disk
The Edgeworth-Kuiper belt (EKB) and its presumed dusty debris is a natural reference for extrsolar debris disks. We re-analyze the current database of known transneptunian objects (TNOs) and employ a
The population of centaurs in the Solar System
Context. Centaurs are objects with perihelia beyond the orbit of Jupiter and semi-major axes inside the orbit of Neptune. They show both cometary and asteroid characteristics, have been observed to
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TLDR
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