Quantifying the impact of the dust torque on the migration of low-mass planets
- Autores
- Guilera, Octavio Miguel; Benítez Llambay, Pablo; Miller Bertolami, Marcelo Miguel; Pessah, Martin E.
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Disk solids are critical in many planet formation processes; however, their effect on planet migration remains largely unexplored. Here we assess this important issue for the first time by building on the systematic measurements of dust torques on an embedded planet by Benitez-Llambay & Pessah. Adopting standard models for the gaseous disk and its solid content, we quantify the impact of the dust torque for a wide range of conditions describing the disk/planet system. We show that the total torque can be positive and reverse inward planet migration for planetary cores with Mp < 10 M⊕. We compute formation tracks for low-mass embryos for conditions usually invoked when modeling planet formation processes. Our most important conclusion is that dust torques can have a significant impact on the migration and formation history of planetary embryos. The most important implications of our findings are as follows. (i) For nominal dust-to-gas mass ratios of epsilon ~0.01, low-mass planets migrate outwards beyond the water ice-line if most of the mass in the solids is in particles with Stokes numbers St ;0.1. (ii) For epsilon ~0.02–0.05, solids with small Stokes numbers, St ; 0.01, can play a dominant role if most of the mass is in those particles. (iii) Dust torques have the potential to enable low-mass planetary cores formed in the inner disk to migrate outwards and act as the seed for massive planets at distances of tens of au.
Fil: Guilera, Octavio Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Benítez Llambay, Pablo. Universidad Adolfo Ibañez; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Pessah, Martin E.. Niels Bohr Institute; Dinamarca - Materia
-
Protoplanetary disks
Planetary-disk interactions
Planet formation
Planetary migration - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/235656
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oai:ri.conicet.gov.ar:11336/235656 |
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Quantifying the impact of the dust torque on the migration of low-mass planetsGuilera, Octavio MiguelBenítez Llambay, PabloMiller Bertolami, Marcelo MiguelPessah, Martin E.Protoplanetary disksPlanetary-disk interactionsPlanet formationPlanetary migrationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Disk solids are critical in many planet formation processes; however, their effect on planet migration remains largely unexplored. Here we assess this important issue for the first time by building on the systematic measurements of dust torques on an embedded planet by Benitez-Llambay & Pessah. Adopting standard models for the gaseous disk and its solid content, we quantify the impact of the dust torque for a wide range of conditions describing the disk/planet system. We show that the total torque can be positive and reverse inward planet migration for planetary cores with Mp < 10 M⊕. We compute formation tracks for low-mass embryos for conditions usually invoked when modeling planet formation processes. Our most important conclusion is that dust torques can have a significant impact on the migration and formation history of planetary embryos. The most important implications of our findings are as follows. (i) For nominal dust-to-gas mass ratios of epsilon ~0.01, low-mass planets migrate outwards beyond the water ice-line if most of the mass in the solids is in particles with Stokes numbers St ;0.1. (ii) For epsilon ~0.02–0.05, solids with small Stokes numbers, St ; 0.01, can play a dominant role if most of the mass is in those particles. (iii) Dust torques have the potential to enable low-mass planetary cores formed in the inner disk to migrate outwards and act as the seed for massive planets at distances of tens of au.Fil: Guilera, Octavio Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Benítez Llambay, Pablo. Universidad Adolfo Ibañez; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Pessah, Martin E.. Niels Bohr Institute; DinamarcaIOP Publishing2023-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/235656Guilera, Octavio Miguel; Benítez Llambay, Pablo; Miller Bertolami, Marcelo Miguel; Pessah, Martin E.; Quantifying the impact of the dust torque on the migration of low-mass planets; IOP Publishing; Astrophysical Journal; 953; 1; 8-2023; 97, 1-170004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/acd2cbinfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/acd2cbinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:23:57Zoai:ri.conicet.gov.ar:11336/235656instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-10 13:23:57.582CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Quantifying the impact of the dust torque on the migration of low-mass planets |
title |
Quantifying the impact of the dust torque on the migration of low-mass planets |
spellingShingle |
Quantifying the impact of the dust torque on the migration of low-mass planets Guilera, Octavio Miguel Protoplanetary disks Planetary-disk interactions Planet formation Planetary migration |
title_short |
Quantifying the impact of the dust torque on the migration of low-mass planets |
title_full |
Quantifying the impact of the dust torque on the migration of low-mass planets |
title_fullStr |
Quantifying the impact of the dust torque on the migration of low-mass planets |
title_full_unstemmed |
Quantifying the impact of the dust torque on the migration of low-mass planets |
title_sort |
Quantifying the impact of the dust torque on the migration of low-mass planets |
dc.creator.none.fl_str_mv |
Guilera, Octavio Miguel Benítez Llambay, Pablo Miller Bertolami, Marcelo Miguel Pessah, Martin E. |
author |
Guilera, Octavio Miguel |
author_facet |
Guilera, Octavio Miguel Benítez Llambay, Pablo Miller Bertolami, Marcelo Miguel Pessah, Martin E. |
author_role |
author |
author2 |
Benítez Llambay, Pablo Miller Bertolami, Marcelo Miguel Pessah, Martin E. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Protoplanetary disks Planetary-disk interactions Planet formation Planetary migration |
topic |
Protoplanetary disks Planetary-disk interactions Planet formation Planetary migration |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Disk solids are critical in many planet formation processes; however, their effect on planet migration remains largely unexplored. Here we assess this important issue for the first time by building on the systematic measurements of dust torques on an embedded planet by Benitez-Llambay & Pessah. Adopting standard models for the gaseous disk and its solid content, we quantify the impact of the dust torque for a wide range of conditions describing the disk/planet system. We show that the total torque can be positive and reverse inward planet migration for planetary cores with Mp < 10 M⊕. We compute formation tracks for low-mass embryos for conditions usually invoked when modeling planet formation processes. Our most important conclusion is that dust torques can have a significant impact on the migration and formation history of planetary embryos. The most important implications of our findings are as follows. (i) For nominal dust-to-gas mass ratios of epsilon ~0.01, low-mass planets migrate outwards beyond the water ice-line if most of the mass in the solids is in particles with Stokes numbers St ;0.1. (ii) For epsilon ~0.02–0.05, solids with small Stokes numbers, St ; 0.01, can play a dominant role if most of the mass is in those particles. (iii) Dust torques have the potential to enable low-mass planetary cores formed in the inner disk to migrate outwards and act as the seed for massive planets at distances of tens of au. Fil: Guilera, Octavio Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Benítez Llambay, Pablo. Universidad Adolfo Ibañez; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Miller Bertolami, Marcelo Miguel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Pessah, Martin E.. Niels Bohr Institute; Dinamarca |
description |
Disk solids are critical in many planet formation processes; however, their effect on planet migration remains largely unexplored. Here we assess this important issue for the first time by building on the systematic measurements of dust torques on an embedded planet by Benitez-Llambay & Pessah. Adopting standard models for the gaseous disk and its solid content, we quantify the impact of the dust torque for a wide range of conditions describing the disk/planet system. We show that the total torque can be positive and reverse inward planet migration for planetary cores with Mp < 10 M⊕. We compute formation tracks for low-mass embryos for conditions usually invoked when modeling planet formation processes. Our most important conclusion is that dust torques can have a significant impact on the migration and formation history of planetary embryos. The most important implications of our findings are as follows. (i) For nominal dust-to-gas mass ratios of epsilon ~0.01, low-mass planets migrate outwards beyond the water ice-line if most of the mass in the solids is in particles with Stokes numbers St ;0.1. (ii) For epsilon ~0.02–0.05, solids with small Stokes numbers, St ; 0.01, can play a dominant role if most of the mass is in those particles. (iii) Dust torques have the potential to enable low-mass planetary cores formed in the inner disk to migrate outwards and act as the seed for massive planets at distances of tens of au. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-08 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/235656 Guilera, Octavio Miguel; Benítez Llambay, Pablo; Miller Bertolami, Marcelo Miguel; Pessah, Martin E.; Quantifying the impact of the dust torque on the migration of low-mass planets; IOP Publishing; Astrophysical Journal; 953; 1; 8-2023; 97, 1-17 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/235656 |
identifier_str_mv |
Guilera, Octavio Miguel; Benítez Llambay, Pablo; Miller Bertolami, Marcelo Miguel; Pessah, Martin E.; Quantifying the impact of the dust torque on the migration of low-mass planets; IOP Publishing; Astrophysical Journal; 953; 1; 8-2023; 97, 1-17 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/acd2cb info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/acd2cb |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1842981326047674368 |
score |
12.48226 |