Mean-Motion Resonances in the Quadrantid Meteoroid Stream and Dynamic Evolution of Dust Trail of (196256) 2003 EH1

TL;DR

This study models mean-motion resonances in the Quadrantid meteoroid stream, revealing multiple planetary resonances that influence dust trail formation, though these effects lack current observational confirmation.

Contribution

The paper introduces detailed numerical models of resonant particles in the Quadrantid stream, identifying specific planetary resonances affecting dust trail dynamics.

Findings

Resonant particles form dust trails far from Earth orbit.

Multiple mean-motion resonances with Venus, Earth, Mars, and Jupiter are identified.

No current observational evidence supports the resonance effects.

Abstract

The paper presents numerical models of mean-motion resonances detected in the Quadrantid meteoroid stream consisting of particles of mass 0.003 to 0.03 g, which helps to prove the presence of the following mean-motion resonances: the 1:9 resonance with Venus, 1:5 resonance with Earth, 1:3 and 3:8 resonances with Mars, and 2:1,7:3, 9:4 resonances with Jupiter. Resonance particles create dust trails far from the Earth orbit. Indeed, there is no observational support for resonant effects in the observed Quadrantid meteoroid stream.