Thermal torque effects on the migration of growing low-mass planets

As planets grow the exchange of angular momentum with the gaseous component of the protoplanetary disc produces a net torque resulting in a variation of the semi-major axis of the planet. For low-mass planets not able to open a gap in the gaseous disc this regime is known as type I migration. Pionee...

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Autores principales: Guilera, Octavio Miguel, Cuello, Nicolás, Montesinos, Matías, Miller Bertolami, Marcelo Miguel, Ronco, María Paula, Cuadra, Jorge, Masset, Frédéric
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2019
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/125057
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id I19-R120-10915-125057
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Planets and satellites: formation
Protoplanetary discs
Planet-disc interactions
spellingShingle Ciencias Astronómicas
Planets and satellites: formation
Protoplanetary discs
Planet-disc interactions
Guilera, Octavio Miguel
Cuello, Nicolás
Montesinos, Matías
Miller Bertolami, Marcelo Miguel
Ronco, María Paula
Cuadra, Jorge
Masset, Frédéric
Thermal torque effects on the migration of growing low-mass planets
topic_facet Ciencias Astronómicas
Planets and satellites: formation
Protoplanetary discs
Planet-disc interactions
description As planets grow the exchange of angular momentum with the gaseous component of the protoplanetary disc produces a net torque resulting in a variation of the semi-major axis of the planet. For low-mass planets not able to open a gap in the gaseous disc this regime is known as type I migration. Pioneer works studied this mechanism in isothermal discs finding fast inward type I migration rates that were unable to reproduce the observed properties of extrasolar planets. In the last years, several improvements have been made in order to extend the study of type I migration rates to non-isothermal discs. Moreover, it was recently shown that if the planet's luminosity due to solid accretion is taken into account, inward migration could be slowed down and even reversed. In this work, we study the planet formation process incorporating, and comparing, updated type I migration rates for non-isothermal discs and the role of planet's luminosity over such rates. We find that the latter can have important effects on planetary evolution, producing a significant outward migration for the growing planets.
format Articulo
Preprint
author Guilera, Octavio Miguel
Cuello, Nicolás
Montesinos, Matías
Miller Bertolami, Marcelo Miguel
Ronco, María Paula
Cuadra, Jorge
Masset, Frédéric
author_facet Guilera, Octavio Miguel
Cuello, Nicolás
Montesinos, Matías
Miller Bertolami, Marcelo Miguel
Ronco, María Paula
Cuadra, Jorge
Masset, Frédéric
author_sort Guilera, Octavio Miguel
title Thermal torque effects on the migration of growing low-mass planets
title_short Thermal torque effects on the migration of growing low-mass planets
title_full Thermal torque effects on the migration of growing low-mass planets
title_fullStr Thermal torque effects on the migration of growing low-mass planets
title_full_unstemmed Thermal torque effects on the migration of growing low-mass planets
title_sort thermal torque effects on the migration of growing low-mass planets
publishDate 2019
url http://sedici.unlp.edu.ar/handle/10915/125057
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AT cuellonicolas thermaltorqueeffectsonthemigrationofgrowinglowmassplanets
AT montesinosmatias thermaltorqueeffectsonthemigrationofgrowinglowmassplanets
AT millerbertolamimarcelomiguel thermaltorqueeffectsonthemigrationofgrowinglowmassplanets
AT roncomariapaula thermaltorqueeffectsonthemigrationofgrowinglowmassplanets
AT cuadrajorge thermaltorqueeffectsonthemigrationofgrowinglowmassplanets
AT massetfrederic thermaltorqueeffectsonthemigrationofgrowinglowmassplanets
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