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      Data analysis of the U–Pb geochronology and Lu–Hf system in zircon and whole-rock Sr, Sm–Nd and Pb isotopic systems for the granitoids of Thailand

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          Abstract

          This data article provides zircon U–Pb and Lu–Hf isotopic information along with whole-rock Sm–Nd, Sr and Pb isotopic geochemistry from granitoids in Thailand. The U–Pb ages are described and the classification of crystallisation and inherited ages are explained. The petrography of the granitoid samples is detailed. The data presented in this article are interpreted and discussed in the research article entitled “Probing into Thailand’s basement: New insights from U–Pb geochronology, Sr, Sm–Nd, Pb and Lu–Hf isotopic systems from granitoids” (Dew et al., 2018).

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          THREE NATURAL ZIRCON STANDARDS FOR U-TH-PB, LU-HF, TRACE ELEMENT AND REE ANALYSES

          M. Wiedenbeck, P. ALLÉ, F. Corfu … (1995)
          Article 0 comments Cited 432 times – based on 0 reviews     Review now
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            Calibration of the Lutetium-Hafnium Clock

            E. Scherer (2001)
            Well-defined constants of radioactive decay are the cornerstone of geochronology and the use of radiogenic isotopes to constrain the time scales and mechanisms of planetary differentiation. Four new determinations of the lutetium-176 decay constant (lambda176Lu) made by calibration against the uranium-lead decay schemes yield a mean value of 1.865 +/- 0.015 x 10(-11) year(-1), in agreement with the two most recent decay-counting experiments. Lutetium-hafnium ages that are based on the previously used lambda176Lu of 1.93 x 10(-11) to 1.94 x 10(-11) year(-1) are thus approximately 4% too young, and the initial hafnium isotope compositions of some of Earth's oldest minerals and rocks become less radiogenic relative to bulk undifferentiated Earth when calculated using the new decay constant. The existence of strongly unradiogenic hafnium in Early Archean and Hadean zircons implies that enriched crustal reservoirs existed on Earth by 4.3 billion years ago and persisted for 200 million years or more. Hence, current models of early terrestrial differentiation need revision.
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              The Hf isotope composition of cratonic mantle: LAM-MC-ICPMS analysis of zircon megacrysts in kimberlites

              W.L. GRIFFIN, N.J. Pearson, E Belousova … (2000)
              Article 0 comments Cited 237 times – based on 0 reviews     Review now
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                Author and article information

                Contributors
                Romana E.C. Dew
                Journal
                Journal ID (nlm-ta): Data Brief
                Journal ID (iso-abbrev): Data Brief
                Title: Data in Brief
                Publisher: Elsevier
                ISSN (Electronic): 2352-3409
                Publication date PMC-release: 09 November 2018
                Publication date Collection: December 2018
                Publication date (Electronic): 09 November 2018
                Volume: 21
                Pages: 1794-1809
                Affiliations
                [a ]Centre for Tectonics, Resources and Exploration (TRaX), Department of Earth Sciences, The University of Adelaide, Adelaide, South Australia 5005, Australia
                [b ]PTTEP, EnCo, Soi 11, GGS, Vibhavadi Rangsit Road, Chatuchak, Bangkok 10900, Thailand
                [c ]Department of Geological Sciences, Chiang Mai University, 239 Huay Kaew Road, Chiang Mai 50200, Thailand
                [d ]Department of Geology, Ghent University, Krijgslaan 281.S8, WE13, 9000 Ghent, Belgium
                [e ]School of Earth and Planetary Science, John de Laeter Centre, TIGeR, Curtin University, Perth, Western Australia, 6102, Australia
                [f ]Basin Analysis and Structural Evolution Special Task Force for Activating Research (BASE STAR), Department of Geology, Faculty of Science, Chulalongkorn University, Bangkok 10330, Thailand
                Author notes
                [* ]Corresponding author. romana.dew@ 123456adelaide.edu.au
                Article
                Publisher ID: S2352-3409(18)31393-3
                DOI: 10.1016/j.dib.2018.10.176
                PMC ID: 6251335
                PubMed ID: 30505918
                SO-VID: 968cd8fd-9ab1-4d9e-bed0-4b4bbffd6617
                Copyright © © 2018 Published by Elsevier Inc.
                License:

                This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).

                History
                Date received : 19 September 2018
                Date revision received : 29 October 2018
                Date accepted : 31 October 2018
                Categories
                Subject: Earth and Planetary Science

                Data availability:

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