Simulations of the Formation of STIPs (Systems of Tightly Packed Inner Planets)
This paper investigates the process of migration of planets of masses ranging from 1 to 20 M⊕ in the protoplanetary disc (Type I Migration) and how it influences the architecture of Planetary Systems.The integrator SyMBA (Duncan et al., 1998 ) was used to generate data for analysis.
Authors
- Pedro H. B. Rosseto
- M. S. Duncan (ORCID: https://orcid.org/0000-0003-4976-6982)
Institutions
- Universidade de Brasília (BR)
Publication Details
- Journal
- Physicae Organum
- Published
- 2025-12-09
- DOI
- https://doi.org/10.26512/2446-564x2017e60659
- Primary Topic
- Astro and Planetary Science
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- Queen's University
- Conselho Nacional de Desenvolvimento Científico e Tecnológico