Subsurface life can modify volatile cycling on a planetary scale

Autores
Giovanelli, D.; Barry, P. H.; Bekaert, D. V.; Chiodi, Agostina Laura; Cordone, A.; Covone, G.; Jessen, G.; Lloyd, K.; de Moor, J. M.; Morrison, S. M.; Schrenk, M. O.; Vitale Brovarone, A.
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The past decade of environmental microbiology has revealed that subsurface environments, both marine and continental, harbor one of the largest ecosystems of our planet, with diversity and biomass rivaling those of the surface. In addition, subsurface life has been recently shown to contribute significantly to the planet’s biogeochemistry, with microbial activity potentially playing an important role in controlling the flux and composition of volatiles recycled between the Earth’s surface and interior, which has broad implications for the search for life beyond our planet. Current efforts to discover extraterrestrial life are focused on planetary bodies with largely inhospitable surfaces, such as Mars, Venus, Europa, Titan, and Enceladus. In these locations, subsurface environments might provide niches of habitability, making the study of deep microbial life a priority for future astrobiological missions. Understanding how volatile elements are exchanged between planetary surfaces and interiors and the role of a subsurface biosphere in altering their composition and flux might provide a tractable target for defining planetary habitability and the detection of subsurface life forms.
Fil: Giovanelli, D.. Università degli Studi di Napoli Federico II; Italia. Tokyo Institute of Technology; Japón. Rutgers University; Estados Unidos. Consiglio Nazionale delle Ricerche; Italia. Woods Hole Oceanographic Institution; Estados Unidos
Fil: Barry, P. H.. Woods Hole Oceanographic Institution; Estados Unidos
Fil: Bekaert, D. V.. Woods Hole Oceanographic Institution; Estados Unidos
Fil: Chiodi, Agostina Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina
Fil: Cordone, A.. Università degli Studi di Napoli Federico II; Italia
Fil: Covone, G.. Università degli Studi di Napoli Federico II; Italia. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Jessen, G.. Universidad Austral de Chile; Chile
Fil: Lloyd, K.. University of Tennessee; Estados Unidos
Fil: de Moor, J. M.. Universidad Nacional; Costa Rica
Fil: Morrison, S. M.. Carnegie Institution For Science; Estados Unidos
Fil: Schrenk, M. O.. Michigan State University; Estados Unidos
Fil: Vitale Brovarone, A.. Alma Mater Studiorum Universit`a Di Bologna; Italia. Sorbonne University; Francia. Museum National d’Histoire Naturelle; Francia
Materia
SUBSURFACE LIFE
VOLATILE CYCLING
ENVIRONMENTAL MICROBIOLOGY
PLANET´S BIOGEOCHEMISTRY
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/183279

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network_name_str CONICET Digital (CONICET)
spelling Subsurface life can modify volatile cycling on a planetary scaleGiovanelli, D.Barry, P. H.Bekaert, D. V.Chiodi, Agostina LauraCordone, A.Covone, G.Jessen, G.Lloyd, K.de Moor, J. M.Morrison, S. M.Schrenk, M. O.Vitale Brovarone, A.SUBSURFACE LIFEVOLATILE CYCLINGENVIRONMENTAL MICROBIOLOGYPLANET´S BIOGEOCHEMISTRYhttps://purl.org/becyt/ford/1.6https://purl.org/becyt/ford/1The past decade of environmental microbiology has revealed that subsurface environments, both marine and continental, harbor one of the largest ecosystems of our planet, with diversity and biomass rivaling those of the surface. In addition, subsurface life has been recently shown to contribute significantly to the planet’s biogeochemistry, with microbial activity potentially playing an important role in controlling the flux and composition of volatiles recycled between the Earth’s surface and interior, which has broad implications for the search for life beyond our planet. Current efforts to discover extraterrestrial life are focused on planetary bodies with largely inhospitable surfaces, such as Mars, Venus, Europa, Titan, and Enceladus. In these locations, subsurface environments might provide niches of habitability, making the study of deep microbial life a priority for future astrobiological missions. Understanding how volatile elements are exchanged between planetary surfaces and interiors and the role of a subsurface biosphere in altering their composition and flux might provide a tractable target for defining planetary habitability and the detection of subsurface life forms.Fil: Giovanelli, D.. Università degli Studi di Napoli Federico II; Italia. Tokyo Institute of Technology; Japón. Rutgers University; Estados Unidos. Consiglio Nazionale delle Ricerche; Italia. Woods Hole Oceanographic Institution; Estados UnidosFil: Barry, P. H.. Woods Hole Oceanographic Institution; Estados UnidosFil: Bekaert, D. V.. Woods Hole Oceanographic Institution; Estados UnidosFil: Chiodi, Agostina Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; ArgentinaFil: Cordone, A.. Università degli Studi di Napoli Federico II; ItaliaFil: Covone, G.. Università degli Studi di Napoli Federico II; Italia. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Jessen, G.. Universidad Austral de Chile; ChileFil: Lloyd, K.. University of Tennessee; Estados UnidosFil: de Moor, J. M.. Universidad Nacional; Costa RicaFil: Morrison, S. M.. Carnegie Institution For Science; Estados UnidosFil: Schrenk, M. O.. Michigan State University; Estados UnidosFil: Vitale Brovarone, A.. Alma Mater Studiorum Universit`a Di Bologna; Italia. Sorbonne University; Francia. Museum National d’Histoire Naturelle; FranciaIstituto Nazionale di Astrofisica2021-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/183279Giovanelli, D.; Barry, P. H.; Bekaert, D. V.; Chiodi, Agostina Laura; Cordone, A.; et al.; Subsurface life can modify volatile cycling on a planetary scale; Istituto Nazionale di Astrofisica; Memorie della Società Astronomica Italiana; 92; 282; 3-2021; 60-631824-016XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://sait.oat.ts.astro.it/MSAIt920221/index.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:59:56Zoai:ri.conicet.gov.ar:11336/183279instacron: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:34982025-09-29 09:59:57.004CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Subsurface life can modify volatile cycling on a planetary scale
title Subsurface life can modify volatile cycling on a planetary scale
spellingShingle Subsurface life can modify volatile cycling on a planetary scale
Giovanelli, D.
SUBSURFACE LIFE
VOLATILE CYCLING
ENVIRONMENTAL MICROBIOLOGY
PLANET´S BIOGEOCHEMISTRY
title_short Subsurface life can modify volatile cycling on a planetary scale
title_full Subsurface life can modify volatile cycling on a planetary scale
title_fullStr Subsurface life can modify volatile cycling on a planetary scale
title_full_unstemmed Subsurface life can modify volatile cycling on a planetary scale
title_sort Subsurface life can modify volatile cycling on a planetary scale
dc.creator.none.fl_str_mv Giovanelli, D.
Barry, P. H.
Bekaert, D. V.
Chiodi, Agostina Laura
Cordone, A.
Covone, G.
Jessen, G.
Lloyd, K.
de Moor, J. M.
Morrison, S. M.
Schrenk, M. O.
Vitale Brovarone, A.
author Giovanelli, D.
author_facet Giovanelli, D.
Barry, P. H.
Bekaert, D. V.
Chiodi, Agostina Laura
Cordone, A.
Covone, G.
Jessen, G.
Lloyd, K.
de Moor, J. M.
Morrison, S. M.
Schrenk, M. O.
Vitale Brovarone, A.
author_role author
author2 Barry, P. H.
Bekaert, D. V.
Chiodi, Agostina Laura
Cordone, A.
Covone, G.
Jessen, G.
Lloyd, K.
de Moor, J. M.
Morrison, S. M.
Schrenk, M. O.
Vitale Brovarone, A.
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv SUBSURFACE LIFE
VOLATILE CYCLING
ENVIRONMENTAL MICROBIOLOGY
PLANET´S BIOGEOCHEMISTRY
topic SUBSURFACE LIFE
VOLATILE CYCLING
ENVIRONMENTAL MICROBIOLOGY
PLANET´S BIOGEOCHEMISTRY
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.6
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The past decade of environmental microbiology has revealed that subsurface environments, both marine and continental, harbor one of the largest ecosystems of our planet, with diversity and biomass rivaling those of the surface. In addition, subsurface life has been recently shown to contribute significantly to the planet’s biogeochemistry, with microbial activity potentially playing an important role in controlling the flux and composition of volatiles recycled between the Earth’s surface and interior, which has broad implications for the search for life beyond our planet. Current efforts to discover extraterrestrial life are focused on planetary bodies with largely inhospitable surfaces, such as Mars, Venus, Europa, Titan, and Enceladus. In these locations, subsurface environments might provide niches of habitability, making the study of deep microbial life a priority for future astrobiological missions. Understanding how volatile elements are exchanged between planetary surfaces and interiors and the role of a subsurface biosphere in altering their composition and flux might provide a tractable target for defining planetary habitability and the detection of subsurface life forms.
Fil: Giovanelli, D.. Università degli Studi di Napoli Federico II; Italia. Tokyo Institute of Technology; Japón. Rutgers University; Estados Unidos. Consiglio Nazionale delle Ricerche; Italia. Woods Hole Oceanographic Institution; Estados Unidos
Fil: Barry, P. H.. Woods Hole Oceanographic Institution; Estados Unidos
Fil: Bekaert, D. V.. Woods Hole Oceanographic Institution; Estados Unidos
Fil: Chiodi, Agostina Laura. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina
Fil: Cordone, A.. Università degli Studi di Napoli Federico II; Italia
Fil: Covone, G.. Università degli Studi di Napoli Federico II; Italia. Istituto Nazionale di Astrofisica; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Jessen, G.. Universidad Austral de Chile; Chile
Fil: Lloyd, K.. University of Tennessee; Estados Unidos
Fil: de Moor, J. M.. Universidad Nacional; Costa Rica
Fil: Morrison, S. M.. Carnegie Institution For Science; Estados Unidos
Fil: Schrenk, M. O.. Michigan State University; Estados Unidos
Fil: Vitale Brovarone, A.. Alma Mater Studiorum Universit`a Di Bologna; Italia. Sorbonne University; Francia. Museum National d’Histoire Naturelle; Francia
description The past decade of environmental microbiology has revealed that subsurface environments, both marine and continental, harbor one of the largest ecosystems of our planet, with diversity and biomass rivaling those of the surface. In addition, subsurface life has been recently shown to contribute significantly to the planet’s biogeochemistry, with microbial activity potentially playing an important role in controlling the flux and composition of volatiles recycled between the Earth’s surface and interior, which has broad implications for the search for life beyond our planet. Current efforts to discover extraterrestrial life are focused on planetary bodies with largely inhospitable surfaces, such as Mars, Venus, Europa, Titan, and Enceladus. In these locations, subsurface environments might provide niches of habitability, making the study of deep microbial life a priority for future astrobiological missions. Understanding how volatile elements are exchanged between planetary surfaces and interiors and the role of a subsurface biosphere in altering their composition and flux might provide a tractable target for defining planetary habitability and the detection of subsurface life forms.
publishDate 2021
dc.date.none.fl_str_mv 2021-03
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/11336/183279
Giovanelli, D.; Barry, P. H.; Bekaert, D. V.; Chiodi, Agostina Laura; Cordone, A.; et al.; Subsurface life can modify volatile cycling on a planetary scale; Istituto Nazionale di Astrofisica; Memorie della Società Astronomica Italiana; 92; 282; 3-2021; 60-63
1824-016X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/183279
identifier_str_mv Giovanelli, D.; Barry, P. H.; Bekaert, D. V.; Chiodi, Agostina Laura; Cordone, A.; et al.; Subsurface life can modify volatile cycling on a planetary scale; Istituto Nazionale di Astrofisica; Memorie della Società Astronomica Italiana; 92; 282; 3-2021; 60-63
1824-016X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://sait.oat.ts.astro.it/MSAIt920221/index.html
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 Istituto Nazionale di Astrofisica
publisher.none.fl_str_mv Istituto Nazionale di Astrofisica
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)
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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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