Dormant Comets Among the Near-Earth Object Population: A Meteor-Based Survey
Quan-Zhi Ye, Peter G. Brown, Petr Pokorn\'y

TL;DR
This study uses meteor radar data to identify dormant comets among near-Earth objects by detecting associated meteor showers, revealing a low dormancy rate and supporting the idea that many JFCs are disrupted or removed.
Contribution
It introduces a novel meteor-based survey method to estimate dormant comet prevalence in the NEO population, providing new statistical insights.
Findings
Detected 5 meteor showers likely linked to dormant comets.
Estimated dormant comet fraction in NEOs is approximately 2%.
Confirmed low dormancy rate supports the disruption hypothesis for JFCs.
Abstract
Dormant comets in the near-Earth object (NEO) population are thought to be involved in the terrestrial accretion of water and organic materials. Identification of dormant comets is difficult as they are observationally indistinguishable from their asteroidal counterparts, however they may have produced dust during their final active stages which potentially are detectable today as weak meteor showers at the Earth. Here we present the result of a reconnaissance survey looking for dormant comets using 13~567~542 meteor orbits measured by the Canadian Meteor Orbit Radar (CMOR). We simulate the dynamical evolution of the hypothetical meteoroid streams originated from 407 near-Earth asteroids in cometary orbits (NEACOs) that resemble orbital characteristics of Jupiter-family comets (JFCs). Out of the 44 hypothetical showers that are predicted to be detectable by CMOR, we identify 5 positive…
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