Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies

ABSTRACT: We report a mechanism capable of reducing (or increasing) stellar activity in binary stars, thereby potentially enhancing (or destroying) circumbinary habitability. In single stars, stellar aggression toward planetary atmospheres causes mass-loss, which is especially detrimental for late-t...

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Autores:
Mason, Paul A.
Zuluaga Callejas, Jorge Iván
Clark, Joni M.
Cuartas Restrepo, Pablo Andrés
Tipo de recurso:
Article of investigation
Fecha de publicación:
2013
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/8532
Acceso en línea:
http://hdl.handle.net/10495/8532
Palabra clave:
Sincronización
Kepler, Johannes, 1571-1630. Sobre los principios de la astronomía
Rotación (física)
Rights
openAccess
License
Atribución-CompartirIgual 2.5 Colombia (CC BY-SA 2.5 CO)
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oai_identifier_str oai:bibliotecadigital.udea.edu.co:10495/8532
network_acronym_str UDEA2
network_name_str Repositorio UdeA
repository_id_str
dc.title.spa.fl_str_mv Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
title Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
spellingShingle Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
Sincronización
Kepler, Johannes, 1571-1630. Sobre los principios de la astronomía
Rotación (física)
title_short Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
title_full Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
title_fullStr Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
title_full_unstemmed Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
title_sort Rotational synchronization may enhance habitability for circumbinary planets : kepler binary case studies
dc.creator.fl_str_mv Mason, Paul A.
Zuluaga Callejas, Jorge Iván
Clark, Joni M.
Cuartas Restrepo, Pablo Andrés
dc.contributor.author.none.fl_str_mv Mason, Paul A.
Zuluaga Callejas, Jorge Iván
Clark, Joni M.
Cuartas Restrepo, Pablo Andrés
dc.subject.none.fl_str_mv Sincronización
Kepler, Johannes, 1571-1630. Sobre los principios de la astronomía
Rotación (física)
topic Sincronización
Kepler, Johannes, 1571-1630. Sobre los principios de la astronomía
Rotación (física)
description ABSTRACT: We report a mechanism capable of reducing (or increasing) stellar activity in binary stars, thereby potentially enhancing (or destroying) circumbinary habitability. In single stars, stellar aggression toward planetary atmospheres causes mass-loss, which is especially detrimental for late-type stars, because habitable zones are very close and activity is long lasting. In binaries, tidal rotational breaking reduces magnetic activity, thus reducing harmful levels of X-ray and ultraviolet (XUV) radiation and stellar mass-loss that are able to erode planetary atmospheres. We study this mechanism for all confirmed circumbinary (p-type) planets. We find that main sequence twins provide minimal flux variation and in some cases improved environments if the stars rotationally synchronize within the first Gyr. Solar-like twins, like Kepler 34 and Kepler 35, provide low habitable zone XUV fluxes and stellar wind pressures. These wide, moist, habitable zones may potentially support multiple habitable planets. Solar-type stars with lower mass companions, like Kepler 47, allow for protected planets over a wide range of secondary masses and binary periods. Kepler 38 and related binaries are marginal cases. Kepler 64 and analogs have dramatically reduced stellar aggression due to synchronization of the primary, but are limited by the short lifetime. Kepler 16 appears to be inhospitable to planets due to extreme XUV flux. These results have important implications for estimates of the number of stellar systems containing habitable planets in the Galaxy and allow for the selection of binaries suitable for follow-up searches for habitable planets.
publishDate 2013
dc.date.issued.none.fl_str_mv 2013
dc.date.accessioned.none.fl_str_mv 2017-10-10T21:10:43Z
dc.date.available.none.fl_str_mv 2017-10-10T21:10:43Z
dc.type.spa.fl_str_mv info:eu-repo/semantics/article
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dc.type.local.spa.fl_str_mv Artículo de investigación
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status_str publishedVersion
dc.identifier.citation.spa.fl_str_mv Mason, P. A., Zuluaga Callejas, J. I., Clark, J. M., & Cuartas Restrepo, P. A. (2013). Rotational synchronization may enhance habitability for circumbinary planets: kepler binary case studies. Astrophysical Journal. 774, 1-8. 10. DOI:1088/2041-8205/774/2/L26
dc.identifier.issn.none.fl_str_mv 0004-637X
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/10495/8532
dc.identifier.doi.none.fl_str_mv 10.1088/2041-8205/774/2/L26
dc.identifier.eissn.none.fl_str_mv 1538-4357
identifier_str_mv Mason, P. A., Zuluaga Callejas, J. I., Clark, J. M., & Cuartas Restrepo, P. A. (2013). Rotational synchronization may enhance habitability for circumbinary planets: kepler binary case studies. Astrophysical Journal. 774, 1-8. 10. DOI:1088/2041-8205/774/2/L26
0004-637X
10.1088/2041-8205/774/2/L26
1538-4357
url http://hdl.handle.net/10495/8532
dc.language.iso.spa.fl_str_mv eng
language eng
dc.rights.*.fl_str_mv Atribución-CompartirIgual 2.5 Colombia (CC BY-SA 2.5 CO)
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rights_invalid_str_mv Atribución-CompartirIgual 2.5 Colombia (CC BY-SA 2.5 CO)
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eu_rights_str_mv openAccess
dc.format.mimetype.spa.fl_str_mv application/pdf
dc.publisher.spa.fl_str_mv Institute of Physics Publishing (IOP)
dc.publisher.group.spa.fl_str_mv Grupo de Fisica y Astrofisica Computacional (FACOM)
dc.publisher.place.spa.fl_str_mv Estados Unidos
institution Universidad de Antioquia
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spelling Mason, Paul A.Zuluaga Callejas, Jorge IvánClark, Joni M.Cuartas Restrepo, Pablo Andrés2017-10-10T21:10:43Z2017-10-10T21:10:43Z2013Mason, P. A., Zuluaga Callejas, J. I., Clark, J. M., & Cuartas Restrepo, P. A. (2013). Rotational synchronization may enhance habitability for circumbinary planets: kepler binary case studies. Astrophysical Journal. 774, 1-8. 10. DOI:1088/2041-8205/774/2/L260004-637Xhttp://hdl.handle.net/10495/853210.1088/2041-8205/774/2/L261538-4357ABSTRACT: We report a mechanism capable of reducing (or increasing) stellar activity in binary stars, thereby potentially enhancing (or destroying) circumbinary habitability. In single stars, stellar aggression toward planetary atmospheres causes mass-loss, which is especially detrimental for late-type stars, because habitable zones are very close and activity is long lasting. In binaries, tidal rotational breaking reduces magnetic activity, thus reducing harmful levels of X-ray and ultraviolet (XUV) radiation and stellar mass-loss that are able to erode planetary atmospheres. We study this mechanism for all confirmed circumbinary (p-type) planets. We find that main sequence twins provide minimal flux variation and in some cases improved environments if the stars rotationally synchronize within the first Gyr. Solar-like twins, like Kepler 34 and Kepler 35, provide low habitable zone XUV fluxes and stellar wind pressures. These wide, moist, habitable zones may potentially support multiple habitable planets. Solar-type stars with lower mass companions, like Kepler 47, allow for protected planets over a wide range of secondary masses and binary periods. Kepler 38 and related binaries are marginal cases. Kepler 64 and analogs have dramatically reduced stellar aggression due to synchronization of the primary, but are limited by the short lifetime. Kepler 16 appears to be inhospitable to planets due to extreme XUV flux. These results have important implications for estimates of the number of stellar systems containing habitable planets in the Galaxy and allow for the selection of binaries suitable for follow-up searches for habitable planets.application/pdfengInstitute of Physics Publishing (IOP)Grupo de Fisica y Astrofisica Computacional (FACOM)Estados Unidosinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_2df8fbb1https://purl.org/redcol/resource_type/ARTArtículo de investigaciónhttp://purl.org/coar/version/c_970fb48d4fbd8a85Atribución-CompartirIgual 2.5 Colombia (CC BY-SA 2.5 CO)info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-sa/2.5/co/http://purl.org/coar/access_right/c_abf2https://creativecommons.org/licenses/by-sa/4.0/SincronizaciónKepler, Johannes, 1571-1630. 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