Four-Dimensional Context of Earth's Supercontinents
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Northwestern Superior Craton Margin, Manitoba: an Overview of Archean
GS-7 Northwestern Superior craton margin, Manitoba: an overview of Archean and Proterozoic episodes of crustal growth, erosion and orogenesis (parts of NTS 54D and 64A) by R.P. Hartlaub1, C.O. Böhm, L.M. Heaman2, and A. Simonetti2 Hartlaub, R.P., Böhm, C.O., Heaman, L.M. and Simonetti, A. 2005: Northwestern Superior craton margin, Manitoba: an overview of Archean and Proterozoic episodes of crustal growth, erosion, and orogenesis (parts of NTS 54D and 64A); in Report of Activities 2005, Manitoba Industry, Economic Development and Mines, Manitoba Geological Survey, p. 54–60. Summary xenocrystic zircon, and in the The northwestern margin of the Superior Province in isotopic signature of Neoarchean Manitoba represents a dynamic boundary zone with good granite bodies (Böhm et al., 2000; potential for magmatic, sedimentary-hosted, and structur- Hartlaub et al., in press). The ALCC extends along the ally controlled mineral deposits. The region has a history Superior margin for at least 50 km, and may have a com- that commences in the early Archean with the formation mon history with other early Archean crustal fragments of the Assean Lake Crustal Complex. This fragment of in northern Quebec and Greenland (Hartlaub et al., in early to middle Archean crust was likely accreted to the press). Superior Province between 2.7 and 2.6 Ga, a major period South of the ALCC, the Split Lake Block repre- of Superior Province amalgamation. Sediments derived sents a variably retrogressed and shear zone–bounded from this amalgamation process were deposited at granulite terrain that is dominated by plutonic rocks and numerous locations along the northwestern margin of mafic granulite (Hartlaub et al., 2003, 2004). -
The Penokean Orogeny in the Lake Superior Region Klaus J
Precambrian Research 157 (2007) 4–25 The Penokean orogeny in the Lake Superior region Klaus J. Schulz ∗, William F. Cannon U.S. Geological Survey, 954 National Center, Reston, VA 20192, USA Received 16 March 2006; received in revised form 1 September 2006; accepted 5 February 2007 Abstract The Penokean orogeny began at about 1880 Ma when an oceanic arc, now the Pembine–Wausau terrane, collided with the southern margin of the Archean Superior craton marking the end of a period of south-directed subduction. The docking of the buoyant craton to the arc resulted in a subduction jump to the south and development of back-arc extension both in the initial arc and adjacent craton margin to the north. A belt of volcanogenic massive sulfide deposits formed in the extending back-arc rift within the arc. Synchronous extension and subsidence of the Superior craton resulted in a broad shallow sea characterized by volcanic grabens (Menominee Group in northern Michigan). The classic Lake Superior banded iron-formations, including those in the Marquette, Gogebic, Mesabi and Gunflint Iron Ranges, formed in that sea. The newly established subduction zone caused continued arc volcanism until about 1850 Ma when a fragment of Archean crust, now the basement of the Marshfield terrane, arrived at the subduction zone. The convergence of Archean blocks of the Superior and Marshfield cratons resulted in the major contractional phase of the Penokean orogeny. Rocks of the Pembine–Wausau arc were thrust northward onto the Superior craton causing subsidence of a foreland basin in which sedimentation began at about 1850 Ma in the south (Baraga Group rocks) and 1835 Ma in the north (Rove and Virginia Formations). -
VAALBARA and TECTONIC EFFECTS of a MEGA IMPACT in the EARLY ARCHEAN 3470 Ma
Large Meteorite Impacts (2003) 4038.pdf VAALBARA AND TECTONIC EFFECTS OF A MEGA IMPACT IN THE EARLY ARCHEAN 3470 Ma T.E. Zegers and A. Ocampo European Space Agency, ESTEC, SCI-SB, Keplerlaan 1, 2201 AZ Noordwijk, [email protected] Abstract The oldest impact related layer recognized on Earth occur in greenstone sequences of the Kaapvaal (South Africa) and Pilbara (Australia) Craton, and have been dated at ca. 3470 Ma (Byerly et al., 2002). The simultaneous occurrence of impact layers now geographically widely separated have been taken to indicate that this was a worldwide phenomena, suggesting a very large impact: 10 to 100 times more massive than the Cretaceous-Tertiary event. However, the remarkable lithostratigraphic and chronostratigraphic similarities between the Pilbara and Kaapvaal Craton have been noted previously for the period between 3.5 and 2.7 Ga (Cheney et al., 1988). Paleomagnetic data from two ultramafic complexes in the Pilbara and Kaapvaal Craton showed that at 2.87 Ga the two cratons could have been part of one larger supercontinent called Vaalbara. New Paleomagnetic results from the older greenstone sequences (3.5 to 3.2 Ga) in the Pilbara and Kaapvaal Craton will be presented. The constructed apparent polar wander path for the two cratons shows remarkable similarities and overlap to a large extent. This suggests that the two cratons were joined for a considerable time during the Archean. Therefore, the coeval impact layers in the two cratons at 3.47 Ga do not necessarily suggest a worldwide phenomena on the present scale of separation of the two cratons. -
Trading Partners: Tectonic Ancestry of Southern Africa and Western Australia, In
Precambrian Research 224 (2013) 11–22 Contents lists available at SciVerse ScienceDirect Precambrian Research journa l homepage: www.elsevier.com/locate/precamres Trading partners: Tectonic ancestry of southern Africa and western Australia, in Archean supercratons Vaalbara and Zimgarn a,b,∗ c d,e f g Aleksey V. Smirnov , David A.D. Evans , Richard E. Ernst , Ulf Söderlund , Zheng-Xiang Li a Department of Geological and Mining Engineering and Sciences, Michigan Technological University, Houghton, MI 49931, USA b Department of Physics, Michigan Technological University, Houghton, MI 49931, USA c Department of Geology and Geophysics, Yale University, New Haven, CT 06520, USA d Ernst Geosciences, Ottawa K1T 3Y2, Canada e Carleton University, Ottawa K1S 5B6, Canada f Department of Earth and Ecosystem Sciences, Division of Geology, Lund University, SE 223 62 Lund, Sweden g Center of Excellence for Core to Crust Fluid Systems, Department of Applied Geology, Curtin University, Perth, WA 6845, Australia a r t i c l e i n f o a b s t r a c t Article history: Original connections among the world’s extant Archean cratons are becoming tractable by the use of Received 26 April 2012 integrated paleomagnetic and geochronologic studies on Paleoproterozoic mafic dyke swarms. Here we Received in revised form ∼ report new high-quality paleomagnetic data from the 2.41 Ga Widgiemooltha dyke swarm of the Yil- 19 September 2012 garn craton in western Australia, confirming earlier results from that unit, in which the primary origin Accepted 21 September 2012 of characteristic remanent magnetization is now confirmed by baked-contact tests. The correspond- Available online xxx ◦ ◦ ◦ ing paleomagnetic pole (10.2 S, 159.2 E, A95 = 7.5 ), in combination with newly available ages on dykes from Zimbabwe, allow for a direct connection between the Zimbabwe and Yilgarn cratons at 2.41 Ga, Keywords: Paleomagnetism with implied connections as early as their cratonization intervals at 2.7–2.6 Ga. -
GSA TODAY North-Central, P
Vol. 9, No. 10 October 1999 INSIDE • 1999 Honorary Fellows, p. 16 • Awards Nominations, p. 18, 20 • 2000 Section Meetings GSA TODAY North-Central, p. 27 A Publication of the Geological Society of America Rocky Mountain, p. 28 Cordilleran, p. 30 Refining Rodinia: Geologic Evidence for the Australia–Western U.S. connection in the Proterozoic Karl E. Karlstrom, [email protected], Stephen S. Harlan*, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131 Michael L. Williams, Department of Geosciences, University of Massachusetts, Amherst, MA, 01003-5820, [email protected] James McLelland, Department of Geology, Colgate University, Hamilton, NY 13346, [email protected] John W. Geissman, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, [email protected] Karl-Inge Åhäll, Earth Sciences Centre, Göteborg University, Box 460, SE-405 30 Göteborg, Sweden, [email protected] ABSTRACT BALTICA Prior to the Grenvillian continent- continent collision at about 1.0 Ga, the southern margin of Laurentia was a long-lived convergent margin that SWEAT TRANSSCANDINAVIAN extended from Greenland to southern W. GOTHIAM California. The truncation of these 1.8–1.0 Ga orogenic belts in southwest- ern and northeastern Laurentia suggests KETILIDEAN that they once extended farther. We propose that Australia contains the con- tinuation of these belts to the southwest LABRADORIAN and that Baltica was the continuation to the northeast. The combined orogenic LAURENTIA system was comparable in -
Lithospheric Architecture Beneath Hudson Bay 10.1002/2015GC005845 Robert W
PUBLICATIONS Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE Lithospheric architecture beneath Hudson Bay 10.1002/2015GC005845 Robert W. Porritt1, Meghan S. Miller1, and Fiona A. Darbyshire2 Special Section: 1 2 The Lithosphere- Department of Earth Sciences, University of Southern California, Los Angeles, California, USA, Centre de recherche asthenosphere System GEOTOP, UniversiteduQu ebec a Montreal, Montreal, Quebec, Canada Key Points: Abstract Hudson Bay overlies some of the thickest Precambrian lithosphere on Earth, whose internal The thick lithosphere of Hudson Bay has significant structural variation structures contain important clues to the earliest workings of plate formation. The terminal collision, the We directly image the thermal Trans-Hudson Orogen, brought together the Western Churchill craton to the northwest and the Superior blanketing on the asthenosphere craton to the southeast. These two Archean cratons along with the Paleo-Proterozoic Trans-Hudson inter- The lithospheric thickness of Hudson Bay is 200–350 km nides, form the core of the North American craton. We use S to P converted wave imaging and absolute shear velocity information from a joint inversion of P to S receiver functions, new ambient noise derived Supporting Information: phase velocities, and teleseismic phase velocities to investigate this region and determine both the thick- Supporting Information S1 ness of the lithosphere and the presence of internal discontinuities. The lithosphere under central Hudson Software S1 Bay approaches 350 km thick but is thinner (200–250 km) around the periphery of the Bay. Furthermore, the amplitude of the LAB conversion from the S receiver functions is unusually large for a craton, suggesting Correspondence to: a large thermal contrast across the LAB, which we interpret as direct evidence of the thermal insulation R. -
Great Lakes Tectonic Zone in Marquette Area, Michigan Implications for Archean Tectonics in North-Central United States
Great Lakes Tectonic Zone in Marquette Area, Michigan Implications for Archean Tectonics in North-Central United States U.S. GEOLOGICAL SURVEY BULLETIN 1904-E AVAILABILITY OF BOOKS AND MAPS OF THE U.S. GEOLOGICAL SURVEY Instructions on ordering publications of the U.S. Geological Survey, along with prices of the last offerings, are given in the cur rent-year issues of the monthly catalog "New Publications of the U.S. Geological Survey." Prices of available U.S. Geological Sur vey publications released prior to the current year are listed in the most recent annual "Price and Availability List." Publications that are listed in various U.S. Geological Survey catalogs (see back inside cover) but not listed in the most recent annual "Price and Availability List" are no longer available. Prices of reports released to the open files are given in the listing "U.S. Geological Survey Open-File Reports," updated month ly, which is for sale in microfiche from the U.S. Geological Survey, Books and Open-File Reports Section, Federal Center, Box 25425, Denver, CO 80225. Reports released through the NTIS may be obtained by writing to the National Technical Information Service, U.S. Department of Commerce, Springfield, VA 22161; please include NTIS report number with inquiry. Order U.S. Geological Survey publications by mail or over the counter from the offices given below. BY MAIL OVER THE COUNTER Books Books Professional Papers, Bulletins, Water-Supply Papers, Techniques of Water-Resources Investigations, Circulars, publications of general in Books -
Paper Number: 5222
Paper Number: 5222 Kaapvaal, Superior and Wyoming: nearest neighbours in supercraton Superia Bleeker, W.1, Chamberlain, K.R.2, Kamo, S.L.3, Hamilton, M.3, Kilian, T.M.4 and Buchan, K.L.1 1Geological Survey of Canada, 601 Booth Street, Ottawa, Canada; email: [email protected]. 2Department of Geology and Geophysics, University of Wyoming, Laramie, USA 3Department of Earth Sciences, University of Toronto, Toronto, Canada 4Department of Geology and Geophysics, Yale University, New Haven, USA ___________________________________________________________________________ Archean cratons embedded in younger continental amalgamations are fragments of late Archean continents or supercratons. Of the ~35 remaining large cratonic fragments, the Superior craton represents one of the larger and better preserved fragments and was a central and defining piece of supercraton Superia [1]. This supercraton, the full extent of which remains to be determined, underwent progressive rifting and breakup during the Paleoproterozoic, spawning ~10 cratonic fragments that were dispersed by plate tectonic movements. Previous work already has shown that Wyoming, “greater Karelia” (i.e. Karelia+Kola), Hearne and a number of other cratons were integral parts of supercraton Superia [e.g., 2, 3]. Specifically, Wyoming craton and Hearne, and “greater Karelia” are fragments that rifted off the southern Superior craton (present reference frame). New work argues that the Kaapvaal craton of southern Africa (and therefore also Pilbara, as part of Vaalbara) was another integral part of Superia, representing the fragment that originated from the re- entrant to the southwest of a combined Superior-Wyoming. A new paleomagnetic interpretation, across more than one time slice, is fully compatible with this interpretation. -
Isotopic Mapping of the Continental Crust: a New Area Selection Tool David Mole, Laurentian University, Sudbury, Canada the Area
Isotopic mapping of the continental crust: A new area selection tool David Mole, Laurentian University, Sudbury, Canada The area selection process is a critical component of exploration targeting. It requires incremental down-scaling, from the planetary-scale, through continent, terrane, and regional scales, using predictive methods, to the belt-scale, where detective methods can be used. Despite the constant search for new tools and technology, the value of new discoveries is currently less than the exploration investment, across a wide range of commodities. This is unsustainable, and demonstrates an urgent need to: (1) push into new search spaces which may be deep, covered, or remote; and (2) develop more effective multi-scale exploration tools for use in these new spaces. Over last 10-15 years, the large-scale spatial application of isotopic data has been shown to effectively image the cryptic architecture of continental areas. Lithospheric and crustal architecture – the framework of major tectonic blocks, terranes and their boundaries – represents a fundamental first-order control on ore deposits and the location of world-class mineral camps. Focused mainly (but not exclusively) within Archean cratons, researchers have constrained the time-resolved lithospheric architecture of large swathes of the continental crust. Champion and Cassidy (2007) used regional Sm-Nd isotopic data to map the crustal architecture of the Yilgarn Craton (Western Australia), and Mole et al. (2013) demonstrated the association between that lithospheric architecture and BIF-hosted iron, orogenic gold, and komatiite-hosted Ni-Cu-PGE systems. Those results demonstrated the underlying control of lithospheric architecture and the potential for isotopic mapping as a greenfields area-selection tool. -
Late Neoarchaean-Palaeoproterozoic Supracrustal Basin-Fills of The
Late Neoarchaean-Palaeoproterozoic supracrustal basin-fills of the Kaapvaal craton: relevance of the supercontinent cycle, the "Great Oxidation Event" and "Snowball Earth"? P.G. Erikssona, N. Lenhardta, D.T. Wrightb, R. Mazumderc and A.J. Bumbya a Department of Geology, University of Pretoria, Pretoria 0002, South Africa b Department of Geology, University of Leicester, University Road, Leicester LE1 7RH c Geological Studies Unit and Fluvial Mechanics Laboratory, Indian Statistical Institute, 203 B.T. Road, Kolkata 700 108, India _____________________________________________________________ Abstract The application of the onset of supercontinentality, the “Great Oxidation Event” (GOE) and the first global-scale glaciation in the Neoarchaean-Palaeoproterozoic as panacea-like events providing a framework or even chronological piercing points in Earth’s history at this time, is questioned. There is no solid evidence that the Kaapvaal craton was part of a larger amalgamation at this time, and its glacigenic record is dominated by deposits supporting the operation of an active hydrological cycle in parallel with glaciation, thereby arguing against the “Snowball Earth Hypothesis”. While the Palaeoproterozoic geological record of Kaapvaal does broadly support the GOE, this postulate itself is being questioned on the basis of isotopic data used as oxygen-proxies, and sedimentological data from extant river systems on the craton argue for a prolongation of the greenhouse palaeo-atmosphere (possibly in parallel with a relative elevation of oxygen levels) which presumably preceded the GOE. The possibility that these widespread events may have been diachronous at the global scale is debated. Keywords: Neoarchaean-Palaeoproterozoic; Kaapvaal craton; sedimentary record; supercontinentality, ca. 2.3 Ga oxidation event, global glaciation _____________________________________________________________________________________ 1. -
A History of Supercontinents on Planet Earth
By Alasdair Wilkins Jan 27, 2011 2:31 PM 47,603 71 Share A history of supercontinents on planet Earth Earth's continents are constantly changing, moving and rearranging themselves over millions of years - affecting Earth's climate and biology. Every few hundred million years, the continents combine to create massive, world-spanning supercontinents. Here's the past and future of Earth's supercontinents. The Basics of Plate Tectonics If we're going to discuss past and future supercontinents, we first need to understand how landmasses can move around and the continents can take on new configurations. Let's start with the basics - rocky planets like Earth have five interior levels: heading outwards, these are the inner core, outer core, mantle, upper mantle, and the crust. The crust and the part of the upper mantle form the lithosphere, a portion of our planet that is basically rigid, solid rock and runs to about 100 kilometers below the planet's surface. Below that is the asthenosphere, which is hot enough that its rocks are more flexible and ductile than those above it. The lithosphere is divided into roughly two dozen major and minor plates, and these plates move very slowly over the almost fluid-like asthenosphere. There are two types of crust: oceanic crust and continental crust. Predictably enough, oceanic crust makes up the ocean beds and are much thinner than their continental counterparts. Plates can be made up of either oceanic or continental crust, or just as often some combination of the two. There are a variety of forces pushing and pulling the plates in various directions, and indeed that's what keeps Earth's crust from being one solid landmass - the interaction of lithosphere and asthenosphere keeps tearing landmasses apart, albeit very, very slowly. -
The Vaalbara Hypotheses Reviewed 1Evans, D.A.D
THE VAALBARA HYPOTHESES REVIEWED 1EVANS, D.A.D., 2MARTIN, D.McB., 2NELSON, D.R., 1POWELL, C.McA., and 1WINGATE, M.T.D. 1Tectonics Special Research Centre, The University of Western Australia, Nedlands, WA, 6907, Australia; 2Geological Survey of Western Australia, Mineral House, 100 Plain St., East Perth, WA, 6004, Australia. Summary present northern Pilbara with eastern Kaapvaal (figure 2b). The The present outlines of Archean cratons commonly show Zegers et al. (1998) Vaalbara model proposes amalgamation by truncation of tectonostratigraphic features, so that wider original 3.1 Ga but perhaps as early as 3.6 Ga, and fragmentation before extents can be inferred. The Kaapvaal and Pilbara cratons share 2.05 Ga. According to isotopic ages alone, a shorter-duration similar 3.6–1.7 Ga geological histories and may have been joined “Zimvaalbara” is suggested by Aspler and Chiaranzelli (1998), for all or part of that interval. Asymmetry of Paleoproterozoic who attributed the widespread 2.8–2.7-Ga igneous activity on foldbelts and coeval foreland basins on both cratons provide Kaapvaal and Pilbara to incipient breakup (also considered by additional, qualitative constraints upon possible reconstructions. Zegers et al., 1998). Although the most reliable paleomagnetic data from ca. 2.8 Ga appear to rule out a direct or even indirect connection at that time, the succeeding billion years’ history lacks pairs of simultaneous and reliable paleomagnetic poles from both blocks, leaving the Paleoproterozoic existence of Vaalbara open to speculation. Introduction Neoarchean and Paleoproterozoic stratigraphic similarities between the Kaapvaal craton in southern Africa, and the Pilbara craton in Western Australia, are so striking that a direct paleogeographic connection during that interval has been proposed and coined “Vaalbara” (Cheney, 1996).