Simulations for Terrestrial Planets Formation
Zhang Niu (1,2), Ji Jianghui (2,3) ((1)Graduate School of Chinese, Academy of Sciences, (2) Purple Mountain Observatory, (3) NAOC)

TL;DR
This study uses simulations to explore terrestrial planet formation after gas dissipation, considering planetary perturbations, initial conditions, and water transfer mechanisms, revealing formation timescales, typical planet counts, and resonance phenomena.
Contribution
It introduces a detailed simulation model incorporating planetary perturbations and initial condition variations to study terrestrial planet formation and water transfer mechanisms.
Findings
Terrestrial planets form within 50 Myr with 60-80% accretion efficiency.
3-4 terrestrial planets typically form inside Jupiter's orbit.
Resonance configurations like 3:2 mean motion resonance are observed.
Abstract
We investigate the formation of terrestrial planets in the late stage of planetary formation using two-planet model. At that time, the protostar has formed for about 3 Myr and the gas disk has dissipated. In the model, the perturbations from Jupiter and Saturn are considered. We also consider variations of the mass of outer planet, and the initial eccentricities and inclinations of embryos and planetesimals. Our results show that, terrestrial planets are formed in 50 Myr, and the accretion rate is about . In each simulation, 3 - 4 terrestrial planets are formed inside "Jupiter" with masses of . In the AU, when the eccentricities of planetesimals are excited, planetesimals are able to accrete material from wide radial direction. The plenty of water material of the terrestrial planet in the Habitable Zone may be transferred from the farther…
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