Accretion rate of extraterrestrial 41Ca in Antarctic snow samples

Autores
Gómez Guzmán, J. M.; Bishop, S.; Faestermann, T.; Famulok, N.; Fimiani, Leticia; Hain, K.; Jahn, S.; Korschinek, G.; Ludwig, P.; Rodrigues Ferreira Maltez, Dario Pablo
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Interplanetary Dust Particles (IDPs) are small grains, generally less than a few hundred micrometers in size. Their main source is the Asteroid Belt, located at 3 AU from the Sun, between Mars and Jupiter. During their flight from the Asteroid Belt to the Earth they are irradiated by galactic and solar cosmic rays (GCR and SCR), thus radionuclides are formed, like 41Ca and 53Mn. Therefore, 41Ca (T1/2 = 1.03 × 105 yr) can be used as a key tracer to determine the accretion rate of IDPs onto the Earth because there are no significant terrestrial sources for this radionuclide. The first step of this study consisted to calculate the production rate of 41Ca in IDPs accreted by the Earth during their travel from the Asteroid Belt. This production rate, used in accordance with the 41Ca/40Ca ratios that will be measured in snow samples from the Antarctica will be used to calculate the amount of extraterrestrial material accreted by the Earth per year. There challenges for this project are, at first, the much longer time for the flight needed by the IDPs to travel from the Asteroid Belt to the Earth in comparison with the 41Ca half-life yields an early saturation for the 41Ca/40Ca ratio, and second, the importance of selecting the correct sampling site to avoid a high influx of natural 40Ca, preventing dilution of the 41Ca/40Ca ratio, the quantity measured by AMS.
Fil: Gómez Guzmán, J. M.. Technische Universitat München; Alemania
Fil: Bishop, S.. Technische Universitat München; Alemania
Fil: Faestermann, T.. Technische Universitat München; Alemania
Fil: Famulok, N.. Technische Universitat München; Alemania
Fil: Fimiani, Leticia. Technische Universitat München; Alemania
Fil: Hain, K.. Technische Universitat München; Alemania
Fil: Jahn, S.. Technische Universitat München; Alemania
Fil: Korschinek, G.. Technische Universitat München; Alemania
Fil: Ludwig, P.. Technische Universitat München; Alemania
Fil: Rodrigues Ferreira Maltez, Dario Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Investigación y Aplicaciones No Nucleares. Gerencia Física (Centro Atómico Constituyentes). Proyecto Tandar; Argentina
Materia
41CA
AMS
INTERPLANETARY DUST
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:11336/98530
Acceder
id CONICETDig_40570ca2b30cd4ea04f1a9f1e112e167
oai_identifier_str oai:ri.conicet.gov.ar:11336/98530
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Accretion rate of extraterrestrial 41Ca in Antarctic snow samplesGómez Guzmán, J. M.Bishop, S.Faestermann, T.Famulok, N.Fimiani, LeticiaHain, K.Jahn, S.Korschinek, G.Ludwig, P.Rodrigues Ferreira Maltez, Dario Pablo41CAAMSINTERPLANETARY DUSThttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Interplanetary Dust Particles (IDPs) are small grains, generally less than a few hundred micrometers in size. Their main source is the Asteroid Belt, located at 3 AU from the Sun, between Mars and Jupiter. During their flight from the Asteroid Belt to the Earth they are irradiated by galactic and solar cosmic rays (GCR and SCR), thus radionuclides are formed, like 41Ca and 53Mn. Therefore, 41Ca (T1/2 = 1.03 × 105 yr) can be used as a key tracer to determine the accretion rate of IDPs onto the Earth because there are no significant terrestrial sources for this radionuclide. The first step of this study consisted to calculate the production rate of 41Ca in IDPs accreted by the Earth during their travel from the Asteroid Belt. This production rate, used in accordance with the 41Ca/40Ca ratios that will be measured in snow samples from the Antarctica will be used to calculate the amount of extraterrestrial material accreted by the Earth per year. There challenges for this project are, at first, the much longer time for the flight needed by the IDPs to travel from the Asteroid Belt to the Earth in comparison with the 41Ca half-life yields an early saturation for the 41Ca/40Ca ratio, and second, the importance of selecting the correct sampling site to avoid a high influx of natural 40Ca, preventing dilution of the 41Ca/40Ca ratio, the quantity measured by AMS.Fil: Gómez Guzmán, J. M.. Technische Universitat München; AlemaniaFil: Bishop, S.. Technische Universitat München; AlemaniaFil: Faestermann, T.. Technische Universitat München; AlemaniaFil: Famulok, N.. Technische Universitat München; AlemaniaFil: Fimiani, Leticia. Technische Universitat München; AlemaniaFil: Hain, K.. Technische Universitat München; AlemaniaFil: Jahn, S.. Technische Universitat München; AlemaniaFil: Korschinek, G.. Technische Universitat München; AlemaniaFil: Ludwig, P.. Technische Universitat München; AlemaniaFil: Rodrigues Ferreira Maltez, Dario Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Investigación y Aplicaciones No Nucleares. Gerencia Física (Centro Atómico Constituyentes). Proyecto Tandar; ArgentinaElsevier Science2015-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/98530Gómez Guzmán, J. M.; Bishop, S.; Faestermann, T.; Famulok, N.; Fimiani, Leticia; et al.; Accretion rate of extraterrestrial 41Ca in Antarctic snow samples; Elsevier Science; Beam Interactions with Materials and Atoms; 361; 10-2015; 620-6260168-583XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.nimb.2015.05.016info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0168583X15004875info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:00:16Zoai:ri.conicet.gov.ar:11336/98530instacron: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 10:00:16.625CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
title Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
spellingShingle Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
Gómez Guzmán, J. M.
41CA
AMS
INTERPLANETARY DUST
title_short Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
title_full Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
title_fullStr Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
title_full_unstemmed Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
title_sort Accretion rate of extraterrestrial 41Ca in Antarctic snow samples
dc.creator.none.fl_str_mv Gómez Guzmán, J. M.
Bishop, S.
Faestermann, T.
Famulok, N.
Fimiani, Leticia
Hain, K.
Jahn, S.
Korschinek, G.
Ludwig, P.
Rodrigues Ferreira Maltez, Dario Pablo
author Gómez Guzmán, J. M.
author_facet Gómez Guzmán, J. M.
Bishop, S.
Faestermann, T.
Famulok, N.
Fimiani, Leticia
Hain, K.
Jahn, S.
Korschinek, G.
Ludwig, P.
Rodrigues Ferreira Maltez, Dario Pablo
author_role author
author2 Bishop, S.
Faestermann, T.
Famulok, N.
Fimiani, Leticia
Hain, K.
Jahn, S.
Korschinek, G.
Ludwig, P.
Rodrigues Ferreira Maltez, Dario Pablo
author2_role author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv 41CA
AMS
INTERPLANETARY DUST
topic 41CA
AMS
INTERPLANETARY DUST
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Interplanetary Dust Particles (IDPs) are small grains, generally less than a few hundred micrometers in size. Their main source is the Asteroid Belt, located at 3 AU from the Sun, between Mars and Jupiter. During their flight from the Asteroid Belt to the Earth they are irradiated by galactic and solar cosmic rays (GCR and SCR), thus radionuclides are formed, like 41Ca and 53Mn. Therefore, 41Ca (T1/2 = 1.03 × 105 yr) can be used as a key tracer to determine the accretion rate of IDPs onto the Earth because there are no significant terrestrial sources for this radionuclide. The first step of this study consisted to calculate the production rate of 41Ca in IDPs accreted by the Earth during their travel from the Asteroid Belt. This production rate, used in accordance with the 41Ca/40Ca ratios that will be measured in snow samples from the Antarctica will be used to calculate the amount of extraterrestrial material accreted by the Earth per year. There challenges for this project are, at first, the much longer time for the flight needed by the IDPs to travel from the Asteroid Belt to the Earth in comparison with the 41Ca half-life yields an early saturation for the 41Ca/40Ca ratio, and second, the importance of selecting the correct sampling site to avoid a high influx of natural 40Ca, preventing dilution of the 41Ca/40Ca ratio, the quantity measured by AMS.
Fil: Gómez Guzmán, J. M.. Technische Universitat München; Alemania
Fil: Bishop, S.. Technische Universitat München; Alemania
Fil: Faestermann, T.. Technische Universitat München; Alemania
Fil: Famulok, N.. Technische Universitat München; Alemania
Fil: Fimiani, Leticia. Technische Universitat München; Alemania
Fil: Hain, K.. Technische Universitat München; Alemania
Fil: Jahn, S.. Technische Universitat München; Alemania
Fil: Korschinek, G.. Technische Universitat München; Alemania
Fil: Ludwig, P.. Technische Universitat München; Alemania
Fil: Rodrigues Ferreira Maltez, Dario Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Investigación y Aplicaciones No Nucleares. Gerencia Física (Centro Atómico Constituyentes). Proyecto Tandar; Argentina
description Interplanetary Dust Particles (IDPs) are small grains, generally less than a few hundred micrometers in size. Their main source is the Asteroid Belt, located at 3 AU from the Sun, between Mars and Jupiter. During their flight from the Asteroid Belt to the Earth they are irradiated by galactic and solar cosmic rays (GCR and SCR), thus radionuclides are formed, like 41Ca and 53Mn. Therefore, 41Ca (T1/2 = 1.03 × 105 yr) can be used as a key tracer to determine the accretion rate of IDPs onto the Earth because there are no significant terrestrial sources for this radionuclide. The first step of this study consisted to calculate the production rate of 41Ca in IDPs accreted by the Earth during their travel from the Asteroid Belt. This production rate, used in accordance with the 41Ca/40Ca ratios that will be measured in snow samples from the Antarctica will be used to calculate the amount of extraterrestrial material accreted by the Earth per year. There challenges for this project are, at first, the much longer time for the flight needed by the IDPs to travel from the Asteroid Belt to the Earth in comparison with the 41Ca half-life yields an early saturation for the 41Ca/40Ca ratio, and second, the importance of selecting the correct sampling site to avoid a high influx of natural 40Ca, preventing dilution of the 41Ca/40Ca ratio, the quantity measured by AMS.
publishDate 2015
dc.date.none.fl_str_mv 2015-10
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/11336/98530
Gómez Guzmán, J. M.; Bishop, S.; Faestermann, T.; Famulok, N.; Fimiani, Leticia; et al.; Accretion rate of extraterrestrial 41Ca in Antarctic snow samples; Elsevier Science; Beam Interactions with Materials and Atoms; 361; 10-2015; 620-626
0168-583X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/98530
identifier_str_mv Gómez Guzmán, J. M.; Bishop, S.; Faestermann, T.; Famulok, N.; Fimiani, Leticia; et al.; Accretion rate of extraterrestrial 41Ca in Antarctic snow samples; Elsevier Science; Beam Interactions with Materials and Atoms; 361; 10-2015; 620-626
0168-583X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nimb.2015.05.016
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0168583X15004875
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 Elsevier Science
publisher.none.fl_str_mv Elsevier Science
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)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
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
_version_ 1844613782016360448
score 13.070432

Publicaciones similares