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  5. Normalized angular momentum deficit: A tool for comparing the violence of the dynamical histories of planetary systems
 

Normalized angular momentum deficit: A tool for comparing the violence of the dynamical histories of planetary systems

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2020
Author(s)
TURRINI, Diego  
•
Zinzi, A.
•
Belinchon, J. A.
DOI
10.1051/0004-6361/201936301
Abstract
Context. Population studies of the orbital characteristics of exoplanets in multi-planet systems have highlighted the existence of an anticorrelation between the average orbital eccentricity of planets and the number of planets of their host system, that is, its multiplicity. This effect was proposed to reflect the varying levels of violence in the dynamical evolution of planetary systems. Aims: Previous work suggested that the relative violence of the dynamical evolution of planetary systems with similar orbital architectures can be compared through the computation of their angular momentum deficit (AMD). We investigated the possibility of using a more general metric to perform analogous comparisons between planetary systems with different orbital architectures. Methods: We considered a modified version of the AMD, the normalized angular momentum deficit (NAMD), and used it to study a sample of 99 multi-planet systems containing both the currently best-characterized extrasolar systems and the solar system, that is, planetary systems with both compact and wide orbital architectures. Results: We verified that the NAMD allows us to compare the violence of the dynamical histories of multi-planet systems with different orbital architectures. We identified an anticorrelation between the NAMD and the multiplicity of the planetary systems, of which the previously observed eccentricity-multiplicity anticorrelation is a reflection. Conclusions: Our results seem to indicate that phases of dynamical instabilities and chaotic evolution are not uncommon among planetary systems. They also suggest that the efficiency of the planetary formation process in producing high-multiplicity systems is likely to be higher than that suggested by their currently known population.
Volume
636
Start page
A53
Uri
http://hdl.handle.net/20.500.12386/35895
Url
http://arxiv.org/abs/2003.05366v2
https://www.aanda.org/articles/aa/full_html/2020/04/aa36301-19/aa36301-19.html
Issn Identifier
0004-6361
Ads BibCode
2020A%26A...636A..53T/
Rights
open.access
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