An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm

<i>Context</i>. The mid-Transit times of an exoplanet may be nonperiodic. The variations in the timing of the transits with respect to a single period, that is, the transit timing variations (TTVs), can sometimes be attributed to perturbations by other exoplanets present in the system, w...

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Autores principales: Carpintero, Daniel Diego, Melita, Mario Daniel
Formato: Articulo
Lenguaje:Inglés
Publicado: 2018
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93848
https://www.aanda.org/articles/aa/abs/2018/12/aa31997-17/aa31997-17.html
Aporte de:
id I19-R120-10915-93848
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Planets and satellites: dynamical evolution and stability
Planets and satellites: individual: Kepler-419b
Planets and satellites: individual: Kepler-419c
spellingShingle Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Planets and satellites: dynamical evolution and stability
Planets and satellites: individual: Kepler-419b
Planets and satellites: individual: Kepler-419c
Carpintero, Daniel Diego
Melita, Mario Daniel
An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm
topic_facet Astronomía
Física
Ciencias Naturales
Ciencias Exactas
Planets and satellites: dynamical evolution and stability
Planets and satellites: individual: Kepler-419b
Planets and satellites: individual: Kepler-419c
description <i>Context</i>. The mid-Transit times of an exoplanet may be nonperiodic. The variations in the timing of the transits with respect to a single period, that is, the transit timing variations (TTVs), can sometimes be attributed to perturbations by other exoplanets present in the system, which may or may not transit the star. <i>Aims</i>. Our aim is to compute the mass and the six orbital elements of an nontransiting exoplanet, given only the central times of transit of the transiting body. We also aim to recover the mass of the star and the mass and orbital elements of the transiting exoplanet, suitably modified in order to decrease the deviation between the observed and the computed transit times by as much as possible. <i>Methods</i>. We have applied our method, based on a genetic algorithm, to the Kepler-419 system. <i>Results</i>. We were able to compute all 14 free parameters of the system, which, when integrated in time, give transits within the observational errors. We also studied the dynamics and the long-Term orbital evolution of the Kepler-419 planetary system as defined by the orbital elements computed by us, in order to determine its stability.
format Articulo
Articulo
author Carpintero, Daniel Diego
Melita, Mario Daniel
author_facet Carpintero, Daniel Diego
Melita, Mario Daniel
author_sort Carpintero, Daniel Diego
title An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm
title_short An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm
title_full An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm
title_fullStr An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm
title_full_unstemmed An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm
title_sort alternative stable solution for the kepler-419 system, obtained with the use of a genetic algorithm
publishDate 2018
url http://sedici.unlp.edu.ar/handle/10915/93848
https://www.aanda.org/articles/aa/abs/2018/12/aa31997-17/aa31997-17.html
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