The end states of long-period comets and the origin of Halley-type comets
Julio A. Fern\'andez, Tabar\'e Gallardo, Juan D. Young

TL;DR
This study models the evolution of long-period comets to understand their end states and the origin of Halley-type comets, revealing that most HTCs originate from Centaurs rather than LPCs, and refining the boundary between these comet types.
Contribution
It introduces a combined dynamical and physico-dynamical model to analyze comet energy distributions and proposes a new boundary between LPCs and HTCs based on energy.
Findings
Most HTCs are not end states of LPC evolution.
Centaurs are a primary source of HTCs.
The LPC-HTC boundary is at an energy of about 0.04 au$^{-1}$.
Abstract
We analyze a sample of 73 old long-period comets (LPCs) (orbital periods yr) with perihelion distances au, discovered in the period 1850-2014. We cloned the observed comets and also added fictitious LPCs with perihelia in the Jupiter's zone. We consider both a purely dynamical evolution and a physico-dynamical one with different physical lifetimes. We can fit the computed energy distribution of comets with au to the observed one only within the energy range au (or periods yr), where the "energy" is taken as the inverse of the semimajor axis , namely . The best results are obtained for physical lifetimes of about 200-300 revolutions (for a comet with a standard au). We find that neither a purely dynamical evolution, nor a physico-dynamical one can reproduce the long tail of larger…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
