Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems
Published Sn isotope data along with 150 new analyses of cassiterite and four granite analyses constrain two major tin isotope fractionation steps associated with (1) separation of tin from the magma/orthomagmatic transitional environment and (2) hydrothermal activity. A distinct Sn isotope differen...
| Autores: | , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/379486 |
| Acceso en línea: | http://hdl.handle.net/10261/379486 |
| Access Level: | acceso abierto |
| Palabra clave: | Sn isotope Tin deposits Metal isotopes |
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Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore SystemsMathur, RyanPowell, WayneYao, JunmingGuimaraes, FredericoCheng, YanboGodfrey, LindaTornos, F.Killick, DavidStephens, JayMao, JingwenSun, MingguangLehmann, BerndSn isotopeTin depositsMetal isotopesPublished Sn isotope data along with 150 new analyses of cassiterite and four granite analyses constrain two major tin isotope fractionation steps associated with (1) separation of tin from the magma/orthomagmatic transitional environment and (2) hydrothermal activity. A distinct Sn isotope difference across deposit type, geological host rocks, and time of ore deposit formation demonstrates that the difference in the mean δ<sup>124</sup>Sn value represents the operation of a unified process. The lower Sn isotope values present in both residual igneous rocks and pegmatite suggest that heavier Sn isotopes were extracted from the system during orthomagmatic fluid separation, likely by F ligands with Sn. Rayleigh distillation models this first F ligand-induced fractionation. The subsequent development of the hydrothermal system is characterized by heavier Sn isotope composition proximal to the intrusion, which persists in spite of Sn isotope fractionating towards isotopically lighter Sn during hydrothermal evolution.The authors appreciate the support of the work from NSF EAR grants 2233425 and 1924177. Yanbo Cheng publishes with permission of the Chief Executive Officer of Geoscience Australia.Peer reviewedMultidisciplinary Digital Publishing InstituteNational Science Foundation (US)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2025202520252025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/379486reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)InglésThe underlying dataset has been published as supplementary material of the article in the publisher platform at DOI https://doi.org/10.3390/geosciences15010028https://doi.org/10.3390/geosciences15010028Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3794862026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| title |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| spellingShingle |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems Mathur, Ryan Sn isotope Tin deposits Metal isotopes |
| title_short |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| title_full |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| title_fullStr |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| title_full_unstemmed |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| title_sort |
Global Sn Isotope Compositions of Cassiterite Identify the Magmatic–Hydrothermal Evolution of Tin Ore Systems |
| dc.creator.none.fl_str_mv |
Mathur, Ryan Powell, Wayne Yao, Junming Guimaraes, Frederico Cheng, Yanbo Godfrey, Linda Tornos, F. Killick, David Stephens, Jay Mao, Jingwen Sun, Mingguang Lehmann, Bernd |
| author |
Mathur, Ryan |
| author_facet |
Mathur, Ryan Powell, Wayne Yao, Junming Guimaraes, Frederico Cheng, Yanbo Godfrey, Linda Tornos, F. Killick, David Stephens, Jay Mao, Jingwen Sun, Mingguang Lehmann, Bernd |
| author_role |
author |
| author2 |
Powell, Wayne Yao, Junming Guimaraes, Frederico Cheng, Yanbo Godfrey, Linda Tornos, F. Killick, David Stephens, Jay Mao, Jingwen Sun, Mingguang Lehmann, Bernd |
| author2_role |
author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
National Science Foundation (US) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Sn isotope Tin deposits Metal isotopes |
| topic |
Sn isotope Tin deposits Metal isotopes |
| description |
Published Sn isotope data along with 150 new analyses of cassiterite and four granite analyses constrain two major tin isotope fractionation steps associated with (1) separation of tin from the magma/orthomagmatic transitional environment and (2) hydrothermal activity. A distinct Sn isotope difference across deposit type, geological host rocks, and time of ore deposit formation demonstrates that the difference in the mean δ<sup>124</sup>Sn value represents the operation of a unified process. The lower Sn isotope values present in both residual igneous rocks and pegmatite suggest that heavier Sn isotopes were extracted from the system during orthomagmatic fluid separation, likely by F ligands with Sn. Rayleigh distillation models this first F ligand-induced fractionation. The subsequent development of the hydrothermal system is characterized by heavier Sn isotope composition proximal to the intrusion, which persists in spite of Sn isotope fractionating towards isotopically lighter Sn during hydrothermal evolution. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025 2025 2025 2025 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/379486 |
| url |
http://hdl.handle.net/10261/379486 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI https://doi.org/10.3390/geosciences15010028 https://doi.org/10.3390/geosciences15010028 Sí |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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Multidisciplinary Digital Publishing Institute |
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Multidisciplinary Digital Publishing Institute |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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