Jumping Neptune Can Explain the Kuiper Belt Kernel
David Nesvorny

TL;DR
This paper proposes that a sudden change in Neptune's orbit during its migration can explain the Kuiper belt kernel, matching observed orbital distributions of icy bodies beyond Neptune.
Contribution
It introduces a novel model where Neptune's semimajor axis change during migration accounts for the Kuiper belt kernel's characteristics.
Findings
Model reproduces the orbital distribution of the kernel.
Resonance sweeping explains the concentration at ~44 AU.
Depletion of bodies beyond 45-47 AU matches observations.
Abstract
The Kuiper belt is a population of icy bodies beyond the orbit of Neptune. A particularly puzzling and up-to-now unexplained feature of the Kuiper belt is the so-called `kernel', a concentration of orbits with semimajor axes a~44 AU, eccentricities e~0.05, and inclinations i<5 deg. Here we show that the Kuiper belt kernel can be explained if Neptune's otherwise smooth migration was interrupted by a discontinuous change of Neptune's semimajor axis when Neptune reached ~28 AU. Before the discontinuity happened, planetesimals located at ~40 AU were swept into Neptune's 2:1 resonance, and were carried with the migrating resonance outwards. The 2:1 resonance was at ~44 AU when Neptune reached ~28 AU. If Neptune's semimajor axis changed by fraction of AU at this point, perhaps because Neptune was scattered off of another planet, the 2:1 population would have been released at ~44 AU, and would…
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