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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/183279
Ver los metadatos del registro completo
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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/ |
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openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Istituto Nazionale di Astrofisica |
publisher.none.fl_str_mv |
Istituto Nazionale di Astrofisica |
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