Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study

Autores
Vigo, Daniel Eduardo; Tuerlinckx, Francis; Scaramal, Mariano; Reimann Baptista, Rafael; Bersenev, Evgeny; Van den Bergh, Omer; Aubert, André E.
Año de publicación
2025
Idioma
español castellano
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Fil: Vigo, Daniel Eduardo. Pontificia Universidad Católica Argentina. Instituto de Investigaciones Biomédicas; Argentina
Fil: Vigo, Daniel Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Vigo, Daniel Eduardo. Katholieke Universiteit Leuven; Bélgica
Fil: Tuerlinckx, Francis. Katholieke Universiteit Leuven; Bélgica
Fil: Scaramal, Mariano. Universidad de San Andrés; Argentina
Fil: Reimann Baptista, Rafael. Pontificia Universidad Católica de Río Grande del Sur; Brasil
Fil: Bersenev, Evgeny. Federal Medical and Biological Agency; Rusia
Fil: Van den Bergh, Omer. Katholieke Universiteit Leuven; Bélgica
Fil: Aubert, André E. Katholieke Universiteit Leuven; Bélgica
Introduction: The aim of this study was to characterize infradian rhythms in heart rate and blood pressure, as well as investigate potential synchronization of these parameters among participants in the Mars500 study. This study involved a 520-day simulated mission to Mars, during which six crew members were confined for the entire duration of the experiment. Methods: The study involved daily measurements of blood pressure and heart rate, taken in the morning and evening for each participant. Mean differences were analyzed using a mixed model design, considering journey stage and time of day as fixed factors, and participant as a random factor. The Lomb-Scargle periodogram was used to identify rhythmic patterns in the data. Significant rhythms were described by fitting a cosine curve using a cosinor model. The level of synchronization between participants’ measurements was assessed by analyzing signal pairs using the Hilbert transform. Phase differences were measured in one-month bins using the gamma parameter. Surrogate data was employed for comparison with the observed data. Gamma differences between bins were evaluated using a mixed model design. Results: All signals showed significant changes over time, and most participants exhibited at least one significant infradian rhythm in the analyzed variables. The primary peaks varied between participants and variables, ranging from 22 days to 520 days. Interestingly, there was a consistent period of 173 days observed in the evening heart rate across all participants. Regarding synchronization, the gamma values of evening heart rate differed from surrogate data in all stages, except during the middle part of the mission. Discussion: The primary finding of this study is the identification of significant infradian rhythms in cardiovascular variables, specifically in evening heart rate, with a shared and synchronized period of 173 days among participants. We propose that affective changes associated with different stages of the mission, along with the cohesive functioning of the crew as a unit, may contribute to these variations.
Fuente
Acta Astronautica. 2025, 229.
Materia
RITMO CIRCADIANO
SISTEMA CARDIOVASCULAR
CONFINAMIENTO
ASTRONAUTAS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
Repositorio Institucional (UCA)
Institución
Pontificia Universidad Católica Argentina
OAI Identificador
oai:ucacris:123456789/19982

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oai_identifier_str oai:ucacris:123456789/19982
network_acronym_str RIUCA
repository_id_str 2585
network_name_str Repositorio Institucional (UCA)
spelling Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement studyVigo, Daniel EduardoTuerlinckx, FrancisScaramal, MarianoReimann Baptista, RafaelBersenev, EvgenyVan den Bergh, OmerAubert, André E.RITMO CIRCADIANOSISTEMA CARDIOVASCULARCONFINAMIENTOASTRONAUTASFil: Vigo, Daniel Eduardo. Pontificia Universidad Católica Argentina. Instituto de Investigaciones Biomédicas; ArgentinaFil: Vigo, Daniel Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Vigo, Daniel Eduardo. Katholieke Universiteit Leuven; BélgicaFil: Tuerlinckx, Francis. Katholieke Universiteit Leuven; BélgicaFil: Scaramal, Mariano. Universidad de San Andrés; ArgentinaFil: Reimann Baptista, Rafael. Pontificia Universidad Católica de Río Grande del Sur; BrasilFil: Bersenev, Evgeny. Federal Medical and Biological Agency; RusiaFil: Van den Bergh, Omer. Katholieke Universiteit Leuven; BélgicaFil: Aubert, André E. Katholieke Universiteit Leuven; BélgicaIntroduction: The aim of this study was to characterize infradian rhythms in heart rate and blood pressure, as well as investigate potential synchronization of these parameters among participants in the Mars500 study. This study involved a 520-day simulated mission to Mars, during which six crew members were confined for the entire duration of the experiment. Methods: The study involved daily measurements of blood pressure and heart rate, taken in the morning and evening for each participant. Mean differences were analyzed using a mixed model design, considering journey stage and time of day as fixed factors, and participant as a random factor. The Lomb-Scargle periodogram was used to identify rhythmic patterns in the data. Significant rhythms were described by fitting a cosine curve using a cosinor model. The level of synchronization between participants’ measurements was assessed by analyzing signal pairs using the Hilbert transform. Phase differences were measured in one-month bins using the gamma parameter. Surrogate data was employed for comparison with the observed data. Gamma differences between bins were evaluated using a mixed model design. Results: All signals showed significant changes over time, and most participants exhibited at least one significant infradian rhythm in the analyzed variables. The primary peaks varied between participants and variables, ranging from 22 days to 520 days. Interestingly, there was a consistent period of 173 days observed in the evening heart rate across all participants. Regarding synchronization, the gamma values of evening heart rate differed from surrogate data in all stages, except during the middle part of the mission. Discussion: The primary finding of this study is the identification of significant infradian rhythms in cardiovascular variables, specifically in evening heart rate, with a shared and synchronized period of 173 days among participants. We propose that affective changes associated with different stages of the mission, along with the cohesive functioning of the crew as a unit, may contribute to these variations.Elsevier2025info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttps://repositorio.uca.edu.ar/handle/123456789/199821879-20300094-576510.1016/j.actaastro.2025.01.060Acta Astronautica. 2025, 229.reponame:Repositorio Institucional (UCA)instname:Pontificia Universidad Católica Argentinaspainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/2025-11-13T10:18:50Zoai:ucacris:123456789/19982instacron:UCAInstitucionalhttps://repositorio.uca.edu.ar/Universidad privadaNo correspondehttps://repositorio.uca.edu.ar/oaiclaudia_fernandez@uca.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:25852025-11-13 10:18:50.639Repositorio Institucional (UCA) - Pontificia Universidad Católica Argentinafalse
dc.title.none.fl_str_mv Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
title Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
spellingShingle Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
Vigo, Daniel Eduardo
RITMO CIRCADIANO
SISTEMA CARDIOVASCULAR
CONFINAMIENTO
ASTRONAUTAS
title_short Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
title_full Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
title_fullStr Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
title_full_unstemmed Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
title_sort Infradian cardiovascular rhythms and between subject cardiovascular coupling in Mars500 prolonged confinement study
dc.creator.none.fl_str_mv Vigo, Daniel Eduardo
Tuerlinckx, Francis
Scaramal, Mariano
Reimann Baptista, Rafael
Bersenev, Evgeny
Van den Bergh, Omer
Aubert, André E.
author Vigo, Daniel Eduardo
author_facet Vigo, Daniel Eduardo
Tuerlinckx, Francis
Scaramal, Mariano
Reimann Baptista, Rafael
Bersenev, Evgeny
Van den Bergh, Omer
Aubert, André E.
author_role author
author2 Tuerlinckx, Francis
Scaramal, Mariano
Reimann Baptista, Rafael
Bersenev, Evgeny
Van den Bergh, Omer
Aubert, André E.
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv RITMO CIRCADIANO
SISTEMA CARDIOVASCULAR
CONFINAMIENTO
ASTRONAUTAS
topic RITMO CIRCADIANO
SISTEMA CARDIOVASCULAR
CONFINAMIENTO
ASTRONAUTAS
dc.description.none.fl_txt_mv Fil: Vigo, Daniel Eduardo. Pontificia Universidad Católica Argentina. Instituto de Investigaciones Biomédicas; Argentina
Fil: Vigo, Daniel Eduardo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Vigo, Daniel Eduardo. Katholieke Universiteit Leuven; Bélgica
Fil: Tuerlinckx, Francis. Katholieke Universiteit Leuven; Bélgica
Fil: Scaramal, Mariano. Universidad de San Andrés; Argentina
Fil: Reimann Baptista, Rafael. Pontificia Universidad Católica de Río Grande del Sur; Brasil
Fil: Bersenev, Evgeny. Federal Medical and Biological Agency; Rusia
Fil: Van den Bergh, Omer. Katholieke Universiteit Leuven; Bélgica
Fil: Aubert, André E. Katholieke Universiteit Leuven; Bélgica
Introduction: The aim of this study was to characterize infradian rhythms in heart rate and blood pressure, as well as investigate potential synchronization of these parameters among participants in the Mars500 study. This study involved a 520-day simulated mission to Mars, during which six crew members were confined for the entire duration of the experiment. Methods: The study involved daily measurements of blood pressure and heart rate, taken in the morning and evening for each participant. Mean differences were analyzed using a mixed model design, considering journey stage and time of day as fixed factors, and participant as a random factor. The Lomb-Scargle periodogram was used to identify rhythmic patterns in the data. Significant rhythms were described by fitting a cosine curve using a cosinor model. The level of synchronization between participants’ measurements was assessed by analyzing signal pairs using the Hilbert transform. Phase differences were measured in one-month bins using the gamma parameter. Surrogate data was employed for comparison with the observed data. Gamma differences between bins were evaluated using a mixed model design. Results: All signals showed significant changes over time, and most participants exhibited at least one significant infradian rhythm in the analyzed variables. The primary peaks varied between participants and variables, ranging from 22 days to 520 days. Interestingly, there was a consistent period of 173 days observed in the evening heart rate across all participants. Regarding synchronization, the gamma values of evening heart rate differed from surrogate data in all stages, except during the middle part of the mission. Discussion: The primary finding of this study is the identification of significant infradian rhythms in cardiovascular variables, specifically in evening heart rate, with a shared and synchronized period of 173 days among participants. We propose that affective changes associated with different stages of the mission, along with the cohesive functioning of the crew as a unit, may contribute to these variations.
description Fil: Vigo, Daniel Eduardo. Pontificia Universidad Católica Argentina. Instituto de Investigaciones Biomédicas; Argentina
publishDate 2025
dc.date.none.fl_str_mv 2025
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 https://repositorio.uca.edu.ar/handle/123456789/19982
1879-2030
0094-5765
10.1016/j.actaastro.2025.01.060
url https://repositorio.uca.edu.ar/handle/123456789/19982
identifier_str_mv 1879-2030
0094-5765
10.1016/j.actaastro.2025.01.060
dc.language.none.fl_str_mv spa
language spa
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Elsevier
publisher.none.fl_str_mv Elsevier
dc.source.none.fl_str_mv Acta Astronautica. 2025, 229.
reponame:Repositorio Institucional (UCA)
instname:Pontificia Universidad Católica Argentina
reponame_str Repositorio Institucional (UCA)
collection Repositorio Institucional (UCA)
instname_str Pontificia Universidad Católica Argentina
repository.name.fl_str_mv Repositorio Institucional (UCA) - Pontificia Universidad Católica Argentina
repository.mail.fl_str_mv claudia_fernandez@uca.edu.ar
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score 13.24909