Semi-analytical Model for the Dynamical Evolution of Planetary Systems via Giant Impacts

In the standard model of terrestrial planet formation, planets are formed through giant impacts of planetary embryos after the dispersal of the protoplanetary gas disk. Traditionally, N -body simulations have been used to investigate this process. However, they are computationally too expensive to g...

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Bibliografski detalji

Glavni autori:	Tadahiro Kimura, Haruka Hoshino, Eiichiro Kokubo, Yuji Matsumoto, Masahiro Ikoma
Format:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2025-01-01
Serija:	The Astrophysical Journal
Teme:	Exoplanet astronomy Exoplanet formation Planet formation Planetary dynamics Planetary system evolution
Online pristup:	https://doi.org/10.3847/1538-4357/ade992
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