Injection of Oort Cloud Comets: The Fundamental Role of Stellar Perturbations
H. Rickman, M. Fouchard, Ch. Froeschl\'e, G.B. Valsecchi

TL;DR
This study uses Monte Carlo simulations to analyze how stellar perturbations and Galactic tides inject comets from the Oort cloud into observable orbits, revealing a significant synergy between these influences that enhances comet injection rates.
Contribution
It provides the first detailed comparison of combined stellar and tidal effects on comet injection, highlighting the critical role of stellar perturbations and their synergy with Galactic tides.
Findings
Stellar perturbations significantly enhance comet injection rates.
Synergy between stellar and tidal effects increases injection beyond individual contributions.
Observable loss cone filling varies from less than 1% to nearly 100% depending on semi-major axis.
Abstract
We present Monte Carlo simulations of the dynamical evolution of the Oort cloud over the age of the Solar System, using an initial sample of one million test comets without any cloning. Our model includes perturbations due to the Galactic tide (radial and vertical) and passing stars. We present the first detailed analysis of the injection mechanism into observable orbits by comparing the complete model with separate models for tidal and stellar perturbations alone. We find that a fundamental role for injecting comets from the region outside the loss cone (perihelion distance q > 15 AU) into observable orbits (q < 5 AU) is played by stellar perturbations. These act in synergy with the tide such that the total injection rate is significantly larger than the sum of the two separate rates. This synergy is as important during comet showers as during quiescent periods and concerns comets with…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Gamma-ray bursts and supernovae
