An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.

Autores
Maizel, Daniela; Ferrero, Marcela Alejandra; Mauas, Pablo Jacobo David
Año de publicación
2015
Idioma
español castellano
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Astrobiology can be defined as a multidisciplinary science that focuses on studies about the origin, evolution, distribution and future of life in the Universe (https://astrobiology. nasa.gov/nai/).In the last 20 years, studies of extrasolar planets have progressed considerably, focusing on the search of planets similar to Earth and in the Habitability Zone (HZ), with a major interest in the search of evidence of life in such environments. It is readily evident that our notion of ?habitability? relies on our limited knowledge of life on Earth. Therefore, in an attempt to find possible forms of life in extraterrestrial systems, it becomes fundamental to enlarge our knowledge about extreme life forms inside our own planet. Such forms of life able to tolerate extreme conditions are mostly known as ?extremophiles? (Caviccioli 2002; Das Sarma, 2006). Some of these organisms have been recently proposed as models for astrobiology studies (Abrevaya et al, 2010; 2011).An interesting case of extremophiles is represented by arsenic- resistant bacteria. Arsenic is a toxic metalloid widely spread in nature. It generally occurs as either arsenate [HAsO42- or As(V)] or arsenite [H2AsO3 or As(III)], the latter species being more toxic than the former. It can be released either by natural weathering of rocks or by anthropogenic sources (Muller et al., 2003). Arsenic is toxic because As and P are similar enough that living organisms attempt this substitution (Wolfe-Simon et al, 2009). Although arsenic is toxic to almost every form of life, it has been previously demonstrated that microorganisms can resist it and also utilize arsenic compounds as a source for growth (Krumova et al., 2008). It has been previously suggested that arsenic-based forms of life could be present on Earth within a ?shadow biosphere?, in similar environments to the ones found outside of the Earth (Davies et al, 2009). These alternative forms of life could currently exist in arsenic-rich environments as much as inside Earth itself as in extraterrestrial systems (Cleland & Copley, 2005; Davies et al, 2009). Even though all known life requires phosphorus (P) in the form of inorganic phosphate, In 2010 Wolfe-Simon et al. reported on a bacterial strain isolated from Mono Lake (California, USA) known as GFAJ-1, which is able to survive in high arsenic concentrations and in the absence of phosphorus. The authors of the work suggested GFAJ-1 as a habitability model in other planets, where different forms of life could be based on arsenic (Wolfe-Simon et al, 2011).Brevibacterium linens AE038-8, is a bacterial strain isolated from As-contaminated groundwater in Tucumán (Argentina), highly resistant to arsenic compounds and capable of growing in extremely low phosphate concentrations, showing a physiology comparable to that of GFAJ-1. It?s recently sequenced genome (Maizel et al, 2015) revealed the presence of arsenate reductase enzymes previously described, which might have evolved from arsenic-rich environments in early life on Earth (Wolfe-Simon et al, 2009). Therefore, we propose strain AE038-8 as an interesting prospect for studies of life in extrasolar planets.
Fil: Maizel, Daniela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Planta Piloto de Procesos Industriales Microbiológicos; Argentina
Fil: Ferrero, Marcela Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Planta Piloto de Procesos Industriales Microbiológicos; Argentina
Fil: Mauas, Pablo Jacobo David. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
58a Reunión Anual de la Asociación Argentina de Astronomía
La Plata
Argentina
Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas
Universidad Nacional de La Plata. Instituto de Astrofíısica de La Plata
Materia
ASTROBIOLOGÍA
ARSENICO
RESISTENCIA
BREVIBACTERIUM
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:11336/195148

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spelling An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.Maizel, DanielaFerrero, Marcela AlejandraMauas, Pablo Jacobo DavidASTROBIOLOGÍAARSENICORESISTENCIABREVIBACTERIUMhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Astrobiology can be defined as a multidisciplinary science that focuses on studies about the origin, evolution, distribution and future of life in the Universe (https://astrobiology. nasa.gov/nai/).In the last 20 years, studies of extrasolar planets have progressed considerably, focusing on the search of planets similar to Earth and in the Habitability Zone (HZ), with a major interest in the search of evidence of life in such environments. It is readily evident that our notion of ?habitability? relies on our limited knowledge of life on Earth. Therefore, in an attempt to find possible forms of life in extraterrestrial systems, it becomes fundamental to enlarge our knowledge about extreme life forms inside our own planet. Such forms of life able to tolerate extreme conditions are mostly known as ?extremophiles? (Caviccioli 2002; Das Sarma, 2006). Some of these organisms have been recently proposed as models for astrobiology studies (Abrevaya et al, 2010; 2011).An interesting case of extremophiles is represented by arsenic- resistant bacteria. Arsenic is a toxic metalloid widely spread in nature. It generally occurs as either arsenate [HAsO42- or As(V)] or arsenite [H2AsO3 or As(III)], the latter species being more toxic than the former. It can be released either by natural weathering of rocks or by anthropogenic sources (Muller et al., 2003). Arsenic is toxic because As and P are similar enough that living organisms attempt this substitution (Wolfe-Simon et al, 2009). Although arsenic is toxic to almost every form of life, it has been previously demonstrated that microorganisms can resist it and also utilize arsenic compounds as a source for growth (Krumova et al., 2008). It has been previously suggested that arsenic-based forms of life could be present on Earth within a ?shadow biosphere?, in similar environments to the ones found outside of the Earth (Davies et al, 2009). These alternative forms of life could currently exist in arsenic-rich environments as much as inside Earth itself as in extraterrestrial systems (Cleland & Copley, 2005; Davies et al, 2009). Even though all known life requires phosphorus (P) in the form of inorganic phosphate, In 2010 Wolfe-Simon et al. reported on a bacterial strain isolated from Mono Lake (California, USA) known as GFAJ-1, which is able to survive in high arsenic concentrations and in the absence of phosphorus. The authors of the work suggested GFAJ-1 as a habitability model in other planets, where different forms of life could be based on arsenic (Wolfe-Simon et al, 2011).Brevibacterium linens AE038-8, is a bacterial strain isolated from As-contaminated groundwater in Tucumán (Argentina), highly resistant to arsenic compounds and capable of growing in extremely low phosphate concentrations, showing a physiology comparable to that of GFAJ-1. It?s recently sequenced genome (Maizel et al, 2015) revealed the presence of arsenate reductase enzymes previously described, which might have evolved from arsenic-rich environments in early life on Earth (Wolfe-Simon et al, 2009). Therefore, we propose strain AE038-8 as an interesting prospect for studies of life in extrasolar planets.Fil: Maizel, Daniela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Planta Piloto de Procesos Industriales Microbiológicos; ArgentinaFil: Ferrero, Marcela Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Planta Piloto de Procesos Industriales Microbiológicos; ArgentinaFil: Mauas, Pablo Jacobo David. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina58a Reunión Anual de la Asociación Argentina de AstronomíaLa PlataArgentinaUniversidad Nacional de La Plata. Facultad de Ciencias Astronómicas y GeofísicasUniversidad Nacional de La Plata. Instituto de Astrofíısica de La PlataUniversidad Nacional de La Plata2015info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectReuniónBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/195148An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.; 58a Reunión Anual de la Asociación Argentina de Astronomía; La Plata; Argentina; 2015; 1-3CONICET DigitalCONICETspainfo:eu-repo/semantics/altIdentifier/url/http://aaa2015.fcaglp.unlp.edu.ar/Archivos/LibroResumenes.pdfNacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:35:20Zoai:ri.conicet.gov.ar:11336/195148instacron: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 09:35:20.945CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
title An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
spellingShingle An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
Maizel, Daniela
ASTROBIOLOGÍA
ARSENICO
RESISTENCIA
BREVIBACTERIUM
title_short An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
title_full An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
title_fullStr An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
title_full_unstemmed An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
title_sort An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.
dc.creator.none.fl_str_mv Maizel, Daniela
Ferrero, Marcela Alejandra
Mauas, Pablo Jacobo David
author Maizel, Daniela
author_facet Maizel, Daniela
Ferrero, Marcela Alejandra
Mauas, Pablo Jacobo David
author_role author
author2 Ferrero, Marcela Alejandra
Mauas, Pablo Jacobo David
author2_role author
author
dc.subject.none.fl_str_mv ASTROBIOLOGÍA
ARSENICO
RESISTENCIA
BREVIBACTERIUM
topic ASTROBIOLOGÍA
ARSENICO
RESISTENCIA
BREVIBACTERIUM
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Astrobiology can be defined as a multidisciplinary science that focuses on studies about the origin, evolution, distribution and future of life in the Universe (https://astrobiology. nasa.gov/nai/).In the last 20 years, studies of extrasolar planets have progressed considerably, focusing on the search of planets similar to Earth and in the Habitability Zone (HZ), with a major interest in the search of evidence of life in such environments. It is readily evident that our notion of ?habitability? relies on our limited knowledge of life on Earth. Therefore, in an attempt to find possible forms of life in extraterrestrial systems, it becomes fundamental to enlarge our knowledge about extreme life forms inside our own planet. Such forms of life able to tolerate extreme conditions are mostly known as ?extremophiles? (Caviccioli 2002; Das Sarma, 2006). Some of these organisms have been recently proposed as models for astrobiology studies (Abrevaya et al, 2010; 2011).An interesting case of extremophiles is represented by arsenic- resistant bacteria. Arsenic is a toxic metalloid widely spread in nature. It generally occurs as either arsenate [HAsO42- or As(V)] or arsenite [H2AsO3 or As(III)], the latter species being more toxic than the former. It can be released either by natural weathering of rocks or by anthropogenic sources (Muller et al., 2003). Arsenic is toxic because As and P are similar enough that living organisms attempt this substitution (Wolfe-Simon et al, 2009). Although arsenic is toxic to almost every form of life, it has been previously demonstrated that microorganisms can resist it and also utilize arsenic compounds as a source for growth (Krumova et al., 2008). It has been previously suggested that arsenic-based forms of life could be present on Earth within a ?shadow biosphere?, in similar environments to the ones found outside of the Earth (Davies et al, 2009). These alternative forms of life could currently exist in arsenic-rich environments as much as inside Earth itself as in extraterrestrial systems (Cleland & Copley, 2005; Davies et al, 2009). Even though all known life requires phosphorus (P) in the form of inorganic phosphate, In 2010 Wolfe-Simon et al. reported on a bacterial strain isolated from Mono Lake (California, USA) known as GFAJ-1, which is able to survive in high arsenic concentrations and in the absence of phosphorus. The authors of the work suggested GFAJ-1 as a habitability model in other planets, where different forms of life could be based on arsenic (Wolfe-Simon et al, 2011).Brevibacterium linens AE038-8, is a bacterial strain isolated from As-contaminated groundwater in Tucumán (Argentina), highly resistant to arsenic compounds and capable of growing in extremely low phosphate concentrations, showing a physiology comparable to that of GFAJ-1. It?s recently sequenced genome (Maizel et al, 2015) revealed the presence of arsenate reductase enzymes previously described, which might have evolved from arsenic-rich environments in early life on Earth (Wolfe-Simon et al, 2009). Therefore, we propose strain AE038-8 as an interesting prospect for studies of life in extrasolar planets.
Fil: Maizel, Daniela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Planta Piloto de Procesos Industriales Microbiológicos; Argentina
Fil: Ferrero, Marcela Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán. Planta Piloto de Procesos Industriales Microbiológicos; Argentina
Fil: Mauas, Pablo Jacobo David. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
58a Reunión Anual de la Asociación Argentina de Astronomía
La Plata
Argentina
Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas
Universidad Nacional de La Plata. Instituto de Astrofíısica de La Plata
description Astrobiology can be defined as a multidisciplinary science that focuses on studies about the origin, evolution, distribution and future of life in the Universe (https://astrobiology. nasa.gov/nai/).In the last 20 years, studies of extrasolar planets have progressed considerably, focusing on the search of planets similar to Earth and in the Habitability Zone (HZ), with a major interest in the search of evidence of life in such environments. It is readily evident that our notion of ?habitability? relies on our limited knowledge of life on Earth. Therefore, in an attempt to find possible forms of life in extraterrestrial systems, it becomes fundamental to enlarge our knowledge about extreme life forms inside our own planet. Such forms of life able to tolerate extreme conditions are mostly known as ?extremophiles? (Caviccioli 2002; Das Sarma, 2006). Some of these organisms have been recently proposed as models for astrobiology studies (Abrevaya et al, 2010; 2011).An interesting case of extremophiles is represented by arsenic- resistant bacteria. Arsenic is a toxic metalloid widely spread in nature. It generally occurs as either arsenate [HAsO42- or As(V)] or arsenite [H2AsO3 or As(III)], the latter species being more toxic than the former. It can be released either by natural weathering of rocks or by anthropogenic sources (Muller et al., 2003). Arsenic is toxic because As and P are similar enough that living organisms attempt this substitution (Wolfe-Simon et al, 2009). Although arsenic is toxic to almost every form of life, it has been previously demonstrated that microorganisms can resist it and also utilize arsenic compounds as a source for growth (Krumova et al., 2008). It has been previously suggested that arsenic-based forms of life could be present on Earth within a ?shadow biosphere?, in similar environments to the ones found outside of the Earth (Davies et al, 2009). These alternative forms of life could currently exist in arsenic-rich environments as much as inside Earth itself as in extraterrestrial systems (Cleland & Copley, 2005; Davies et al, 2009). Even though all known life requires phosphorus (P) in the form of inorganic phosphate, In 2010 Wolfe-Simon et al. reported on a bacterial strain isolated from Mono Lake (California, USA) known as GFAJ-1, which is able to survive in high arsenic concentrations and in the absence of phosphorus. The authors of the work suggested GFAJ-1 as a habitability model in other planets, where different forms of life could be based on arsenic (Wolfe-Simon et al, 2011).Brevibacterium linens AE038-8, is a bacterial strain isolated from As-contaminated groundwater in Tucumán (Argentina), highly resistant to arsenic compounds and capable of growing in extremely low phosphate concentrations, showing a physiology comparable to that of GFAJ-1. It?s recently sequenced genome (Maizel et al, 2015) revealed the presence of arsenate reductase enzymes previously described, which might have evolved from arsenic-rich environments in early life on Earth (Wolfe-Simon et al, 2009). Therefore, we propose strain AE038-8 as an interesting prospect for studies of life in extrasolar planets.
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An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.; 58a Reunión Anual de la Asociación Argentina de Astronomía; La Plata; Argentina; 2015; 1-3
CONICET Digital
CONICET
url http://hdl.handle.net/11336/195148
identifier_str_mv An arsenic resistant bacteria isolated in Tucumán, Argentina, as a model microorganism for astrobiology studies.; 58a Reunión Anual de la Asociación Argentina de Astronomía; La Plata; Argentina; 2015; 1-3
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