Li Isotopes and Trace Elements As a Petrogenetic Tracer in Zircon: Insights from Archean Ttgs and Sanukitoids

Total Page:16

File Type:pdf, Size:1020Kb

Li Isotopes and Trace Elements As a Petrogenetic Tracer in Zircon: Insights from Archean Ttgs and Sanukitoids Contrib Mineral Petrol (2012) 163:745–768 DOI 10.1007/s00410-011-0697-1 ORIGINAL PAPER Li isotopes and trace elements as a petrogenetic tracer in zircon: insights from Archean TTGs and sanukitoids Anne-Sophie Bouvier • Takayuki Ushikubo • Noriko T. Kita • Aaron J. Cavosie • Reinhard Kozdon • John W. Valley Received: 7 March 2011 / Accepted: 14 September 2011 / Published online: 2 October 2011 Ó Springer-Verlag 2011 Abstract We report d7Li, Li abundance ([Li]), and other granitoids is significantly higher than from zircons in trace elements measured by ion probe in igneous zircons primitive magmas in oceanic crust. TTG zircons have d7Li from TTG (tonalite, trondhjemite, and granodiorite) and (3 ± 8%) and d18O in the range of primitive mantle- sanukitoid plutons from the Superior Province (Canada) in derived magmas. Sanukitoid zircons have average d7Li order to characterize Li in zircons from typical Archean (7 ± 8%) and d18O higher than those of TTGs supporting continental crust. These data are compared with detrital genesis by melting of fluid-metasomatized mantle wedge. zircons from the Jack Hills (Western Australia) with U–Pb The Li systematics in sanukitoid and TTG zircons indicate ages greater than 3.9 Ga for which parent rock type is not that high [Li] in pre-3.9-Ga Jack Hills detrital zircons is a known. Most of the TTG and sanukitoid zircon domains primary igneous composition and suggests the growth in preserve typical igneous REE patterns and CL zoning. [Li] proto-continental crust in magmas similar to Archean ranges from 0.5 to 79 ppm, typical of [Li] in continental granitoids. zircons. Atomic ratios of (Y ? REE)/(Li ? P) average 1.0 ± 0.7 (2SD) for zircons with magmatic composition Keywords Zircon Á Trace elements Á Lithium isotopes Á preserved, supporting the hypothesis that Li is interstitial SIMS Á Jack Hills Á TTG Á Sanukitoid and charge compensates substitution of trivalent cations. This substitution results in a relatively slow rate of Li diffusion. The d7Li and trace element data constrain the Introduction genesis of TTGs and sanukitoids. [Li] in zircons from Zircons are a retentive accessory mineral in many rocks. They are extensively used for U–Pb geochronology, giving Communicated by F. Poitrasson. useful information about tectonic events and related pro- Electronic supplementary material The online version of this cesses (e.g., Davis et al. 2003). Zircons also give valuable article (doi:10.1007/s00410-011-0697-1) contains supplementary geochemical information from oxygen isotope ratios and material, which is available to authorized users. trace elements (Hoskin and Schaltegger 2003; Valley 2003). Magmatic d18O values are generally preserved in A.-S. Bouvier (&) Á T. Ushikubo Á N. T. Kita Á R. Kozdon Á J. W. Valley non-metamict zircons, even through high-grade metamor- WiscSIMS, Department of Geoscience, University of Wisconsin, phism and anatexis (Page et al. 2007; Valley et al. 2005; Madison, WI 53706, USA Watson and Cherniak 1997). Grimes et al. (2007) used e-mail: [email protected] trace elements to show that zircons from continental crust Present Address: can be distinguished from oceanic crust. Recently, Li A.-S. Bouvier content ([Li]) and d7Li in zircons have been reported Swedish Museum of Natural History, 10405 Stockholm, Sweden (Grimes et al. 2011; Li et al. 2011; Ushikubo et al. 2008) showing that Li is useful for characterizing a zircon’s A. J. Cavosie Department of Geology, University of Puerto Rico, Mayagu¨ez, parent rock. However, interpreting the significance of [Li] PR 00681, USA and d7Li in zircons requires better understanding of the 123 746 Contrib Mineral Petrol (2012) 163:745–768 possible effects of alteration in Li and d7Li distribution in Speer 1982). Possible substitutions are summarized in zircon, Li substitution mechanisms, and Li diffusion rates Table 1. Some substitutions are simple, such as tetravalent in zircon. Hf, U, Th, Ti, and Sn ions that could directly substitute for Here, we report the analysis of d7Li, [Li], and other trace Zr?4, whereas other elements require a coupled substitution elements in zircons coupled to imaging for well-studied for charge balance. Finch et al. (2001) and Hanchar et al. igneous suites. This is the first study reporting analyses of (2001) suggested that Li substitutes on an interstitial site, d7Li, associated with 23 trace elements (Li, P, Ca, Ti, V, charge-balancing REE and Y (see Table 1), leading to a Fe, Y, REE, U, and Th) in single analysis pits in zircon. couple substitution as follows: Due to intracrystalline zoning, such correlated analyses are Li1þ þ ðÞY þ REE 3þ¼ Zr4þ þ h ð2Þ necessary to test the proposed Li substitutions in zircons. ðinterstitialÞ ðÞinterstitial We chose igneous zircons from TTGs and sanukitoids When converted to atomic proportions, each ppm of Li with ages ranging from 2.7 to 3.0 Ga, which are typical (at. wt * 7 amu) compensates for over twenty times its Archean granitoids (e.g., King et al. 1998). The selected weight in REE (at. wt * 150 amu) in Eq. (2). In this case, TTG and sanukitoid zircons are from the Superior Province if Li and P compensate REE, the ratio defining these two 18 (Canada), and d O(Zrc) and U–Pb ages are reported coupled substitutions, [(Y ? REE)/(Li ? P)]atomic, should IV 1? elsewhere (Davis et al. 2005; King et al. 1998). The use of be 1 (Ushikubo et al. 2008). Because Li has a larger 4? well-described zircons with known parent rocks allows ionic radius than Si (Shannon 1976), Li is unlikely to be VIII VIII testing the potential of [Li] and d7Li as petrogenetic trac- incorporated in Si sites. Alternatively, Li could fit Zr ers. The differences in trace elements, Li, and d7Li between sites, associated with 3 interstitial Li for charge compen- zircons from four TTG and four sanukitoid plutons are sation (Eq. 3). Li could also be 100% interstitial for charge discussed in terms of their different petrogenesis. These compensation of Zr, if an eightfold vacancy can exist data are also compared to Archean detrital zircons from the (Eq. 4). Jack Hills (Western Australia) that are older than 3.9 Ga VIII þ þ VIII 4þ h Li þ 3LiðintersitialÞ ¼ Zr þ 3 ðinterstitialÞ ð3Þ (up to 4.35 Ga) and for which parent rock type is uncertain. þ VIII h 4þ h 4LiðinterstitialÞ þ ¼ Zr þ 4 ðinterstitialÞ ð4Þ Li substitution in zircons Li substitution in natural zircons was recently discovered While Li is a mobile element in many processes, zircon to vary by over 5 orders of magnitude, from \2 ppb to appears to be highly retentive (Ushikubo et al. 2008); 250 ppm (Ushikubo et al. 2008). Zircons from primitive however, Li exchange in zircon is not well understood. The magmas, the mantle, and ocean crust are low in [Li] mechanism of lithium substitution in zircon affects chem- (kimberlite megacrysts \2 ppb, mid-ocean ridge gabbro ical diffusion rates and must be evaluated before it can be \10 ppb, and mid-ocean ridge plagiogranite \ 100 ppb), interpreted as reflecting magmatic compositions. Zircon is whereas zircons from continental crust have significantly higher Li contents (typically 1–100 ppm, Barth and an orthosilicate in which isolated SiO4 tetrahedra shares Wooden 2010; Grimes et al. 2011; Ushikubo et al. 2008). corners and edges with distorted ZrO8 polyhedra. The zircon crystal structure incorporates a wide range of trace elements, including Li, P, Y, Ti, Hf, U, Th, and REE (Finch Li isotopic fractionation et al. 2001; Hanchar et al. 2001; Hoskin and Schaltegger 2003). Incorporation of REE in zircon is commonly Fresh igneous rocks from the mantle have d7Li(whole assumed to be a ‘‘xenotime-type’’ substitution, because of rock) = 3.8 ± 1.5% (Chan et al. 2002a, b; Jeffcoate et al. the high [P] in many zircons and because zircon is iso- 2007; Magna et al. 2006; Seitz et al. 2004; Tomascak et al. 7 structural with xenotime (YPO4). The charge-balanced 2008), whereas seawater has very high d Li (*31%; Chan substitution is as follows: and Edmond 1988; Millot et al. 2004; Tomascak 2004; You and Chan 1996). Li isotope fractionation during ðÞY þ REE 3þþP5þ ¼ Zr4þ þ Si4þ ð1Þ fluid–rock interaction causes up to 50% variation in d7Li, If xenotime-type substitution solely governs the REE with products of subaerial weathering as low as -20% incorporation in zircons, P5? and REE3? compensate and (Chan and Edmond 1988; Chan et al. 1992, 2002a; Pist- [(Y ? REE)/P]atomic should be 1. However, numerous iner and Henderson 2003; Rudnick and Ionov 2007; studies have observed an excess of total REE compared Seyfried et al. 1998; Teng et al. 2008). Continental crust 7 with P (i.e., [(Y ? REE)/P]atomic [ 1), indicating that at has an average d Li(WR) of ?1.7% (Teng et al. 2009), least one other substitutional mechanism occurs (Cavosie making d7Li a potential tracer of continental alteration et al. 2006; Hinton and Upton 1991; Pidgeon et al. 1998; and weathering. 123 Contrib Mineral Petrol (2012) 163:745–768 747 Table 1 Substitution in zircons Element Equations References Xenotime substitution Y3? (Y ? REE)3? ? P5? = Zr4? ? Si4? Simple substitutions (OH)4 (OH)4 = SiO4 Frondel (1953) Hf4? Hf4? = Zr4? Frondel (1953) U4?,Th4?,Ti4?,Sn4? (U, Th, Ti, Sn)4? = Zr4? Frondel (1953) Coupled substitutions Li? 1þ 3þ 4þ Finch et al. (2001), Hanchar et al. (2001) LiðinterstitialÞ þ REE ¼ Zr - n? - 4? 4- a (OH) M ? n(OH) ? (4 - n)H2O = Zr ? (SiO4) Caruba and Iacconi (1983) Mg2?,Fe2? 2þ 3þ 5þ 4þ 4þ Hoskin et al. (2000) ðÞMg; Fe ðinterstitialÞþ3YðÞ; REE þP ¼ 3Zr þ Si Al3?,Fe3? 3þ 3þ 5þ 4þ 4þ Hoskin et al.
Recommended publications
  • Eoarchean Crustal Evolution of the Jack Hills Zircon Source and Loss of Hadean Crust
    Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 146 (2014) 27–42 www.elsevier.com/locate/gca Eoarchean crustal evolution of the Jack Hills zircon source and loss of Hadean crust Elizabeth A. Bell ⇑, T. Mark Harrison, Issaku E. Kohl, Edward D. Young Dept. of Earth, Planetary, and Space Sciences, UCLA, United States Received 10 March 2014; accepted in revised form 18 September 2014; available online 30 September 2014 Abstract Given the global dearth of Hadean (>4 Ga) rocks, 4.4–4.0 Ga detrital zircons from Jack Hills, Narryer Gneiss Complex (Yilgarn Craton, Western Australia) constitute our best archive of early terrestrial materials. Previous Lu–Hf investigations of these zircons suggested that felsic (low Lu/Hf) crust formation began by 4.4 to 4.5 Ga and continued for several hundred million years with evidence of the least radiogenic Hf component persisting until at least 4 Ga. However, evidence for the involvement of Hadean materials in later crustal evolution is sparse, and even in the detrital Jack Hills zircon population, the most unradiogenic, ancient isotopic signals have not been definitively identified in the younger (<3.9 Ga) rock and zircon record. Here we show Lu–Hf data from <4 Ga Jack Hills detrital zircons that document a significant and previously unknown transition in Yilgarn Craton crustal evolution between 3.9 and 3.7 Ga. The zircon source region evolved largely by internal reworking through the period 4.0–3.8 Ga, and the most ancient and unradiogenic components of the crust are mostly missing from the record after 4 Ga.
    [Show full text]
  • Temporal Variation in Relative Zircon Abundance Throughout Earth History
    Letter Geochemical Perspectives Letters magma crystallisation, crust production, and even crustal composition (Condie et al., 2009; Cawood et al., 2013; Parman, 2015; Lee et al., 2016). However, quantity of zircon is not a direct substitute for quantity of magma or crust. Instead, zircon © 2017 European Association of Geochemistry abundance in the igneous record is a function of magma composition, which is both spatially and temporally heterogeneous. Moreover, due to the high closure temperatures of the U-Th/Pb and U-series systems, ages from these geochro- Temporal variation in relative zircon nometers exclusively date zircon crystallisation (Schoene, 2014), which need not abundance throughout Earth history coincide with the crystallisation of other silicate minerals. The temperature Tsat at which zircon saturates in an igneous magma can C.B. Keller1,2,3*, P. Boehnke4,5, B. Schoene3 be accurately predicted by an empirical equation of the form Zr a zircon = ln + bM + c T Zr sat melt Abstract doi: 10.7185/geochemlet.1721 where a, b, and c are constants, [Zr] is zirconium concentration, and M is a Zircon is the preeminent chronometer of deep time on Earth, informing models of crustal compositional measure of magma polymerisation defined on a molar basis as growth and providing our only direct window into the Hadean Eon. However, the quantity of zircon crystallised per unit mass of magma is highly variable, complicating interpreta- Na + K + 2 Ca tion of the terrestrial zircon record. Here we combine zircon saturation simulations with a M = dataset of ~52,000 igneous whole rock geochemical analyses to quantify secular variation in Al ∗ Si relative zircon abundance throughout Earth history.
    [Show full text]
  • The Geochronology and Geochemistry of Zircon As Evidence for the Reconcentration of REE in the Triassic Period in the Chungju Area, South Korea
    minerals Article The Geochronology and Geochemistry of Zircon as Evidence for the Reconcentration of REE in the Triassic Period in the Chungju Area, South Korea Sang-Gun No 1,* and Maeng-Eon Park 2 1 Mineral Resources Development Research Center, Korea Institute of Geoscience and Mineral Resources, Daejeon 34132, Korea 2 Department of Earth Environmental Science, Pukyong National University, Busan 48513, Korea; [email protected] * Correspondence: [email protected]; Tel.: +82-10-9348-7807 Received: 1 November 2019; Accepted: 2 January 2020; Published: 5 January 2020 Abstract: The Chungju rare-earth element (REE) deposit is located in the central part of the Okcheon Metamorphic Belt (OMB) in the Southern Korean Peninsula and research on REE mineralization in the Gyemyeongsan Formation has been continuous since the first report in 1989. The genesis of the REE mineralization that occurred in the Gyemyeongsan Formation has been reported by previous researchers; theories include the fractional crystallization of alkali magma, magmatic hydrothermal alteration, and recurrent mineralization during metamorphism. In the Gyemyeongsan Formation, we discovered an allanite-rich vein that displays the paragenetic relationship of quartz, allanite, and zircon, and we investigated the chemistry and chronology of zircon obtained from this vein. We analyzed the zircon’s chemistry with an electron probe X-ray micro analyzer (EPMA) and laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS). The grain size of the zircon is as large as 50 µm and has an inherited core (up to 15 µm) and micrometer-sized sector zoning (up to several micrometers in size). In a previous study, the zircon ages were not obtained because the grain size was too small to analyze.
    [Show full text]
  • RESEARCH Oxygen Isotopes in Detrital Zircons
    RESEARCH Oxygen isotopes in detrital zircons: Insight into crustal recycling during the evolution of the Greenland Shield C.L. Kirkland1,3*†, M.J. Whitehouse1, V. Pease2, and M. Van Kranendonk3,4 1SWEDISH MUSEUM OF NATURAL HISTORY, BOX 50007, SE-104 05 STOCKHOLM, SWEDEN 2DEPARTMENT OF GEOLOGY & GEOCHEMISTRY, STOCKHOLM UNIVERSITY, SE-106 91 STOCKHOLM, SWEDEN 3GEOLOGICAL SURVEY OF WESTERN AUSTRALIA, DEPARTMENT OF MINES AND PETROLEUM, 100 PLAIN STREET, EAST PERTH, WA 6004, AUSTRALIA 4SCHOOL OF EARTH AND GEOGRAPHICAL SCIENCES, UNIVERSITY OF WESTERN AUSTRALIA, 35 STIRLING HWY., CRAWLEY WA 6009, AUSTRALIA ABSTRACT Insight into the interactions between crust and hydrosphere, through the protracted evolution of the Greenland Shield, can be provided by oxygen isotopes in the mineral remnants of its denuded crust. Detrital zircons with ages of 3900 Ma to 900 Ma found within an arkosic sand- stone dike of the Neoproterozoic (?Marinoan) Mørænesø Formation, North Greenland, provide a time-integrated record of the evolution of part of the Greenland Shield. These zircon grains are derived from a wide variety of sources in northeastern Laurentia, including Paleo- proterozoic and older detritus from the Committee-Melville orogen, the Ellesmere-Inglefi eld mobile belt, and the subice continuation of the δ18 Victoria Fjord complex. Archean zircon crystals have a more restricted range of OSMOW values (between 7.2‰ and 9.0‰ relative to stan- δ18 dard mean ocean water [SMOW]) in comparison to Paleoproterozoic 1800–2100 Ma grains, which display signifi cant variation in OSMOW (6.8‰–10.4‰). These data refl ect differences in crustal evolution between the Archean and Proterozoic Earth. Through time, remelting or reworking of high δ18O materials has become more important, consistent with the progressive emergence of buoyant, cratonized continental lithosphere.
    [Show full text]
  • Earth's Oldest Rocks
    Chapter 12 The Oldest Terrestrial Mineral Record: Thirty Years of Research on Hadean Zircon From Jack Hills, Western Australia Aaron J. Cavosie1, John W. Valley2 and Simon A. Wilde3 1Curtin University, Perth, WA, Australia; 2University of WisconsineMadison, Madison, WI, United States; 3Curtin University of Technology, Perth, WA, Australia Chapter Outline 1. Introduction 255 3.4.1 Lithium 266 2. Jack Hills Metasedimentary Rocks 256 3.4.2 Ti Thermometry 266 2.1 Age of Deposition 257 3.4.3 Rare Earth Elements, Yttrium and Phosphorous 266 2.2 Metamorphism 258 3.4.4 Other Trace Elements (Al, Sc, Sm/Nd, Xe) 267 2.3 Geology of Adjacent Rocks 258 3.5 Hafnium Isotopic Compositions 267 3. Studies of Jack Hills Zircon 259 3.6 Mineral Inclusion Studies 268 3.1 Images of Jack Hills Zircon 259 4. Early Earth Processes Recorded by Jack Hills Zircon 270 3.2 Age of the Hadean Zircon Population 259 4.1 Derivation of Jack Hills Zircon From Early Mafic 3.2.1 The UePb Story 259 Crust (εHf) 270 3.2.2 U Abundance, Radiation Damage, and Pb Loss 261 4.2 Existence of >4300 Ma Granitoid 270 3.2.3 The Oldest Grains in the Jack Hills 262 4.3 Significance of Surface Alteration on the Early Earth 271 3.2.4 Distribution of Hadean Grains 264 4.4 Impact Events Recorded in Jack Hills Zircon? 271 3.3 Oxygen Isotopes 264 Acknowledgments 273 3.4 Trace Elements 266 References 273 1. INTRODUCTION Little is known of the early Earth because of the absence of a rock record for the first 500 million years after accretion.
    [Show full text]
  • Heterogeneous Hadean Crust with Ambient Mantle Affinity Recorded in Detrital Zircons of the Green Sandstone Bed, South Africa
    Heterogeneous Hadean crust with ambient mantle affinity recorded in detrital zircons of the Green Sandstone Bed, South Africa Nadja Drabona,1,2, Benjamin L. Byerlyb,3, Gary R. Byerlyc, Joseph L. Woodend,4, C. Brenhin Kellere, and Donald R. Lowea aDepartment of Geological Sciences, Stanford University, Stanford, CA 94305; bDepartment of Earth Sciences, University of California, Santa Barbara, CA 93106; cDepartment of Geology and Geophysics, Louisiana State University, Baton Rouge, LA 70803; dPrivate address, Marietta, GA 30064; and eDepartment of Earth Sciences, Dartmouth College, Hanover, NH 03755 Edited by Albrecht W. Hofmann, Max Planck Institute for Chemistry, Mainz, Germany, and approved January 4, 2021 (received for review March 10, 2020) The nature of Earth’s earliest crust and the processes by which it While the crustal rocks in which Hadean zircon formed have formed remain major issues in Precambrian geology. Due to the been lost, the trace and rare earth element (REE) geochemistry of absence of a rock record older than ∼4.02 Ga, the only direct re- these zircons can be used to characterize their parental magma cord of the Hadean is from rare detrital zircon and that largely compositions. Zircon crystallizes as a ubiquitous accessory mineral from a single area: the Jack Hills and Mount Narryer region of in silica-rich, differentiated magmas formed in a number of crustal Western Australia. Here, we report on the geochemistry of environments. Since zircon compositions are influenced by varia- Hadean detrital zircons as old as 4.15 Ga from the newly discov- tions in melt composition, coexisting mineral assemblage, and trace ered Green Sandstone Bed in the Barberton greenstone belt, element partitioning as a function of magmatic processes, temper- South Africa.
    [Show full text]
  • Geochemical Signatures and Magmatic Stability of Impact Produced Zircon
    Early Solar System Impact Bombardment II (2012) 4041.pdf Geochemical Signatures and Magmatic Stability of Impact Produced Zircon. M. M. Wielicki1, T. M. Harrison1 and A. K. Schmitt1 1Department of Earth and Space Sciences, University of California, Los Angeles, 595 Charles E. Young Drive East, Los Angeles, CA 90095 ([email protected]). Introduction: The impact history of the early so- ritance and leaving open the possibility that the pub- lar system, including Earth and the Moon, remains a lished ages reflect post-impact effects. contreversial issue within planetary science. Since the Inherited zircon, from the target rock, was present Apollo program, the concept of a late heavy bombard- in impactites from Vredefort and will be depth profiled ment (LHB) or lunar catalclysm has been hypothe- to determine if overgrowth rims dating to the impact sized. The LHB is a spike in the flux of bolides within event are present on these grains. the inner solar system from 3.8-4.0 Ga that would have Ti-in-zircon thermometry. Applying the Ti-in- resurfaced the Moon and ~30% of Earth. Evidence for zircon thermometer to impact proiduced zircons from such an event exists in widespread isotopic resetting of known terrestrial impact sites and comparing results to Apollo samples at ~3.9 Ga [1] as well as K-Ar ages of the remarkably low temperatures [~680°C; 7] asso- lunar meteorites [2]. ciated with Hadean zircons could provide evidence in Recent studies have suggested that the mineral zir- assessing a possible impact origin for these ancient con (ZrSiO4) has the potential to record large scale grains.
    [Show full text]
  • In Situ U-Pb, O and Hf Isotopic Compositions of Zircon and Olivine from Eoarchaean Rocks, West Greenland: New Insights to Making Old Crust
    University of Wollongong Research Online Faculty of Science - Papers (Archive) Faculty of Science, Medicine and Health January 2009 In situ U-Pb, O and Hf isotopic compositions of zircon and olivine from Eoarchaean rocks, West Greenland: new insights to making old crust Joe Hiess NERC Isotope Geosciences Laboratory Vickie C. Bennett Australian National University Allen P. Nutman University of Wollongong, [email protected] Ian S. Williams Follow this and additional works at: https://ro.uow.edu.au/scipapers Part of the Life Sciences Commons, Physical Sciences and Mathematics Commons, and the Social and Behavioral Sciences Commons Recommended Citation Hiess, Joe; Bennett, Vickie C.; Nutman, Allen P.; and Williams, Ian S.: In situ U-Pb, O and Hf isotopic compositions of zircon and olivine from Eoarchaean rocks, West Greenland: new insights to making old crust 2009, 4489-4516. https://ro.uow.edu.au/scipapers/985 Research Online is the open access institutional repository for the University of Wollongong. For further information contact the UOW Library: [email protected] In situ U-Pb, O and Hf isotopic compositions of zircon and olivine from Eoarchaean rocks, West Greenland: new insights to making old crust Abstract The sources and petrogenetic processes that generated some of the Earth's oldest continental crust have been more tightly constrained via an integrated, in situ (U-Pb, O and Hf) isotopic approach. The minerals analysed were representative zircon from four Eoarchaean TTG tonalites and two felsic volcanic rocks, and olivine from one harzburgite/dunite of the Itsaq Gneiss Complex (IGC), southern West Greenland. The samples were carefully chosen from localities with least migmatisation, metasomatism and strain.
    [Show full text]
  • Hadean Geodynamics and the Nature of Early Continental Crust
    Precambrian Research 359 (2021) 106178 Contents lists available at ScienceDirect Precambrian Research journal homepage: www.elsevier.com/locate/precamres Invited Review Article Hadean geodynamics and the nature of early continental crust Jun Korenaga Department of Earth and Planetary Sciences, Yale University, P.O. Box 208109, New Haven, CT 06520-8109, USA ARTICLE INFO ABSTRACT Keywords: Reconstructing Earth history during the Hadean defiesthe traditional rock-based approach in geology. Given the Plate tectonics extremely limited locality of Hadean zircons, some indirect approach needs to be employed to gain a global Early atmosphere perspective on the Hadean Earth. In this review, two promising approaches are considered jointly. One is to Magma ocean better constrain the evolution of continental crust, which helps to definethe global tectonic environment because Continental growth generating a massive amount of felsic continental crust is difficultwithout plate tectonics. The other is to better understand the solidification of a putative magma ocean and its consequences, as the end of magma ocean so­ lidification marks the beginning of subsolidus mantle convection. On the basis of recent developments in these two subjects, along with geodynamical consideration, a new perspective for early Earth evolution is presented, which starts with rapid plate tectonics made possible by a chemically heterogeneous mantle and gradually shifts to a more modern-style plate tectonics with a homogeneous mantle. The theoretical and observational stance of this new hypothesis is discussed in conjunction with a critical review of existing proposals for early Earth dy­ namics, such as stagnant lid convection, sagduction, episodic and intermittent subduction, and heat pipe. One unique feature of the new hypothesis is its potential to explain the evolution of nearly all components in the Earth system, including the atmosphere, the oceans, the crust, the mantle, and the core, in a geodynamically sensible manner.
    [Show full text]
  • THE HADEAN EARTH. TM Harrison
    id21254828 pdfMachine by Broadgun Software - a great PDF writer! - a great PDF creator! - http://www.pdfmachine.com http://www.broadgun.com Lunar and Planetary Science XXXVIII (2007) 2033.pdf THE HADEAN EARTH. T. M. Harrison (Institute of Geophysics and Planetary Physcis & Dept. of Earth and Space Sciences, UCLA, Los Angeles, CA 90095, U.S.A.) and Project MtREE. Introduction: The Hadean Eon (4.5-4.0 Ga) is the water was available during prograde melting relatively ’s su dark age of Earth history; there is no known rock re- close to the Earth rface. cord from this period. However, detrital zircons as old Origin of the continental crust: The long favored as nearly 4.4 Ga from the Jack Hills, Western Austra- paradigm for continent formation is that initial growth lia, offer unprecedented insights into this formative was forestalled until ~4 Ga and then grew slowly until phase of Earth history. Investigations using these an- present day. However, a minority view [3] has per- cient zircons suggest that they formed by a variety of sisted that continental crust was widespread during the processes involving a hydrosphere within ~200 m.y. of Hadean. Initial 176Hf/177Hf ratios of Jack Hills zircons planetary accretion and challenge the view that conti- ranging in age from 3.96 to 4.35 Ga show surprisingly nental and hydrosphere formation were frustrated by large positive and negative isotope heterogeneities in- meteorite bombardment and basaltic igneous activity dicating that a major differentiation of the silicate Earth until ~4 Ga. occurred at ~4.5 Ga [4]. A likely consequence of this The Mission to Really Early Earth (MtREE): differentiation is the formation of continental crust with MtREE is an international consortium using Hadean a volume of similar order to the present, possibly via zircons to investigate the earliest evolution of the at- the mechanism described by Morse [5].
    [Show full text]
  • High-Precision Oxygen Isotope Analysis of Picogram Samples Reveals 2 Μm Gradients and Slow Diffusion in Zircon
    American Mineralogist, Volume 92, pages 1772–1775, 2007 LETTER High-precision oxygen isotope analysis of picogram samples reveals 2 μm gradients and slow diffusion in zircon F. ZEB PAGE,1,* T. USHIKUBO,1 N.T. KITA,1 L.R. RICIPUTI,2 AND J.W. VALLEY1 1Department of Geology and Geophysics, University of Wisconsin—Madison, 1215 W. Dayton St., Madison, Wisconsin 53706, U.S.A. 2Oak Ridge National Laboratory, P.O. Box 2008, MS6375, Oak Ridge, Tennessee 37831-6375, U.S.A. ABSTRACT Ion microprobe analysis with a sub-micrometer diameter spot reveals a sharp, 2 μm gradient in oxygen isotope ratio proving that oxygen diffusion in zircon is slow even under prolonged high-grade metamorphism. The data are consistent with an oxygen diffusion coefÞ cient of 10–23.5±1 cm2/s. Fur- thermore, this gradient is found in a zircon that contains clear textural evidence of recrystallization in nearby regions. This Þ nding shows that through careful textural and chemical analysis, primary information can be extracted from a zircon that has also undergone partial recrystallization. The oxygen isotope ratios found in zircon have been used to infer magmatic and pre-magmatic histories, including the presence of liquid water on the surface of earliest Earth. Recently, these interpretations have been questioned with the assertion that zircon may not retain its primary oxygen isotope signature through metamorphism. The slow diffusion conÞ rmed by these results supports interpretations that assume preservation of magmatic compositions. Keywords: Ion microprobe, SIMS, zircon, diffusion, oxygen isotopes, stable isotopes, granulites facies, migmatites INTRODUCTION Several studies have shown that zircons preserve primary 18 Oxygen isotopic ratios are constant for primitive magmatic magmatic values of δ O through episodes of metamorphism, rocks from the Earth’s mantle, but can be highly fractionated by magmatism, and hydrothermal alteration (Valley et al.
    [Show full text]
  • High Sensitivity Mapping of Ti Distributions in Hadean Zircons ⁎ T
    Earth and Planetary Science Letters 261 (2007) 9–19 www.elsevier.com/locate/epsl High sensitivity mapping of Ti distributions in Hadean zircons ⁎ T. Mark Harrison , Axel K. Schmitt Department of Earth and Space Sciences and Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, CA 90095, USA Received 16 February 2007; received in revised form 4 May 2007; accepted 7 May 2007 Available online 13 May 2007 Editor: R.W. Carlson Abstract Detrital zircons as old as nearly 4.4 Ga from the Jack Hills, Western Australia, offer possible insights into a phase of Earth history for which there exists no known rock record. Ti concentrations of Hadean zircons indicate a spectrum of crystallization temperatures that range from a cluster at ca. 680 °C to apparent values exceeding 1200 °C. The low temperature peak has been interpreted to indicate the existence of ‘wet’ melting conditions during the Hadean, but alternate views have been advanced. We have developed methods for quantitative ion imaging of titanium in zircons using positive and negative secondary ions, produced respectively under bombardment of O− and Cs+, that permit detailed insights regarding Ti concentration distributions. Each approach has particular advantages that tradeoff in terms of sensitivity, ultimate lateral resolution, and reproducibility. Coupled with high resolution spot analyses, these ion images show that Ti contents greater than about 20 ppm in the Jack Hills zircons are associated with cracks or other crystal imperfections and that virtually all of the high apparent temperatures (i.e., N800 °C) yet obtained are suspect for contamination by Ti extraneous to the zircon.
    [Show full text]