Helium and carbon isotopes in thermal waters of the Jalisco block, Mexico

The Jalisco block is a geologically and tectonically complex part of western Mexico. It is considered a distinct crustal unit bounded toward the mainland by rifting and toward the Pacific ocean by the SW section of the Mid-America trench, a contact between the subducting Rivera plate and the contine...

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Detalhes bibliográficos
Autores: Taran, Yuri, Inguaggiato, Salvatore, Varley, Nicholas, Capasso, Giorgio, Favara, Rocco
Tipo de documento: artigo
Estado:Versão publicada
Data de publicação:2002
País:México
Recursos:UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO
Repositório:Geofísica Internacional
Idioma:espanhol
OAI Identifier:oai:revistagi.geofisica.unam.mx:article/852
Acesso em linha:http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/852
Access Level:Acceso aberto
Palavra-chave:Bloque de Jalisco
isótopos de helio y de carbono
geoquímica de agua y gas, tectónica
Jalisco Block
helium isotopes
carbon isotopes
water and gas geochemistry
tectonics
Descrição
Resumo:The Jalisco block is a geologically and tectonically complex part of western Mexico. It is considered a distinct crustal unit bounded toward the mainland by rifting and toward the Pacific ocean by the SW section of the Mid-America trench, a contact between the subducting Rivera plate and the continent. On the basis of chemical, helium, and carbon isotopic analyses of 37 groups of thermal springs widely distributed over the Jalisco block, several major tectonic environments can be distinguished. The highest R= 3He/4He ratios with R/Ra (Ra being the atmospheric 3He/4He ratio) approaching MORB values were observed along the Trans-Mexican Volcanic Belt (TMVB) and within the Colima volcanic complex. For springs in the inner part of the block and close to the Pacific coast, including submarine springs at Punta de Mita, typical values were much lower, with R/Ra down to 0.4 . A negative correlation between 3He/4He and δ13C of CO2 is suggested to be the result of coupling between radiogenic He and CO2 formed by oxidation of organic-rich sediments. C/3He ratios vary from ~109 for TMVB, typical for volatiles released from the mantle, to > 1011 thus suggesting a substantial addition of carbon from the crust.