Geochemical Evidence in the Northeast Lau Basin for Subduction
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Cenozoic Changes in Pacific Absolute Plate Motion A
CENOZOIC CHANGES IN PACIFIC ABSOLUTE PLATE MOTION A THESIS SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI`I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN GEOLOGY AND GEOPHYSICS DECEMBER 2003 By Nile Akel Kevis Sterling Thesis Committee: Paul Wessel, Chairperson Loren Kroenke Fred Duennebier We certify that we have read this thesis and that, in our opinion, it is satisfactory in scope and quality as a thesis for the degree of Master of Science in Geology and Geophysics. THESIS COMMITTEE Chairperson ii Abstract Using the polygonal finite rotation method (PFRM) in conjunction with the hotspot- ting technique, a model of Pacific absolute plate motion (APM) from 65 Ma to the present has been created. This model is based primarily on the Hawaiian-Emperor and Louisville hotspot trails but also incorporates the Cobb, Bowie, Kodiak, Foundation, Caroline, Mar- quesas and Pitcairn hotspot trails. Using this model, distinct changes in Pacific APM have been identified at 48, 27, 23, 18, 12 and 6 Ma. These changes are reflected as kinks in the linear trends of Pacific hotspot trails. The sense of motion and timing of a number of circum-Pacific tectonic events appear to be correlated with these changes in Pacific APM. With the model and discussion presented here it is suggested that Pacific hotpots are fixed with respect to one another and with respect to the mantle. If they are moving as some paleomagnetic results suggest, they must be moving coherently in response to large-scale mantle flow. iii List of Tables 4.1 Initial hotspot locations . -
Predicted Path for Hotspot Tracks Off South America Since Paleocene Times: Tectonic Implications of Ridge-Trench Collision Along the Andean Margin
Gondwana Research 64 (2018) 216–234 Contents lists available at ScienceDirect Gondwana Research journal homepage: www.elsevier.com/locate/gr Predicted path for hotspot tracks off South America since Paleocene times: Tectonic implications of ridge-trench collision along the Andean margin Juan Pablo Bello-González a,⁎, Eduardo Contreras-Reyes b,CésarArriagadaa a Laboratorio de Paleomagnetismo, Departamento de Geología, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago, Chile b Departamento de Geofísica, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago, Chile article info abstract Article history: Hotspots are generated by partial melting due to hot plumes rising within the Earth's mantle, and when tectonic Received 12 January 2018 plates move relative to the plume source, hotspot tracks form. Off South America, the oceanic Nazca Plate hosts a Received in revised form 20 July 2018 large population of hotspot tracks. Examples include seamounts formed far from the Pacific-Nazca spreading cen- Accepted 23 July 2018 ter (“off-ridge” seamounts), such as the Juan Fernández Ridge (Juan Fernández hotspot), the Taltal Ridge (San Available online 20 September 2018 Félix hotspot), and the Copiapó Ridge (Caldera hotspot). These hotspot tracks are characterized by a rough and fi “ Handling Editor: T. Gerya discontinuous topography. Other examples include seamounts formed near the East Paci c Rise (EPR) ( on- ridge” seamounts), such as the Nazca Ridge (Salas y Gómez hotspot) and Easter Seamount Chain (Easter hotspot), Keywords: and the Iquique Ridge (Foundation hotspot). These oceanic ridges developed a relatively smooth and broad mor- Hotspot phology. Here, we present a plate reconstruction of these six oceanic hotspot tracks since the Paleocene, provid- Volcanism ing a kinematic model of ridge-continental margin collision. -
Chemical Systematics of an Intermediate Spreading Ridge: the Pacific-Antarctic Ridge Between 56°S and 66°S
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 105, NO. B2, PAGES 2915-2936, FEBRUARY 10, 2000 Chemical systematics of an intermediate spreading ridge: The Pacific-Antarctic Ridge between 56°S and 66°S Ivan Vlastélic,I,2 Laure DOSSO,I Henri Bougault/ Daniel Aslanian,3 Louis Géli,3 Joël Etoubleau,3 Marcel Bohn,1 Jean-Louis Joron,4 and Claire Bollinger l Abstract. Axial bathymetry, major/trace elements, and isotopes suggest that the Pacific-Antarctic Ridge (PAR) between 56°S and 66°S is devoid of any hotspot influence. PAR (56-66°S) samples 144 have in average lower 87Sr/86Sr and 143 Nd/ Nd and higher 206 PbP04 Pb than northern Pacific l11id ocean ridge basalts (MORB), and also than MORB From the other oceans. The high variability of pb isotopic ratios (compared to Sr and Nd) can be due to either a general high ~l (I-IIMU) (high U/Pb) affïnity of the southern Pacific upper mantle or to a mantle event first recorded in time by Pb isotopes. Compiling the results ofthis study with those From the PAR between 53°S and 57°S gives a continuous vie~ of mantle characteristics fr~m sOl~th ,Pitman. Fracture Z?ne (FZ) to . Vacquier FZ, representll1g about 3000 km of spreadll1g aXIs. [he latitude ofUdmtsev FZ (56°S) IS a limit between, to the narth, a domain with large geochemical variations and, to the south, one with small variations. The spreading rate has intermediate values (54 mm/yr at 66°S to 74 mm/yr at 56°S) which increase along the PAR, while the axial morphology changes from valley to dome. -
Non-Hawaiian Lithostratigraphy of Louisville Seamounts and the Formation of High-Latitude Oceanic Islands and Guyots
Non-Hawaiian lithostratigraphy of Louisville seamounts and the formation of high-latitude oceanic islands and guyots David M. Buchsa,⁎, Rebecca Williamsb, Shin-ichi Sanoc, V. Paul Wrightd a Cardiff University, UK b University of Hull, UK c Fukui Prefectural Dinosaur Museum, Japan d National Museum of Wales, UK This is an author accepted manuscript for an article published in Journal of Volcanology and Geothermal Research, doi: 10.1016/j.jvolgeores.2017.12.019. ABSTRACT Guyots are large seamounts with a flat summit that is generally believed to form due to constructional biogenic and/or erosional processes during the formation of volcanic islands. However, despite their large abundance in the oceans, there are still very few direct constraints on the nature and formation of guyots, in particular those formed at high latitude that lack a thick cap of shallow-marine carbonate rocks. It is largely accepted based on geophysical constraints and surficial observations/sampling that the summit platform of these guyots is shaped by wave abrasion during post-volcanic subsidence of volcanic islands. Here we provide novel constraints on this hypothesis and the summit geology of guyots with a lithostratigraphic analysis of cores from three Louisville seamounts (South Pacific) collected during Expedition 330 of the Integrated Ocean Drilling Program (IODP). Thirteen lithofacies of sedimentary and volcanic deposits are described, which include facies not previously recognized on the top of guyots, and offer a new insight into the formation of high-latitude oceanic islands on a fast- moving plate. Our results reveal that the lithostratigraphy of Louisville seamounts preserves a very consistent record of the formation and drowning of volcanic islands, with from bottom to top: (i) volcaniclastic sequences with abundant lava-fed delta deposits, (ii) submarine to subaerial shield lava flows, (iii) post-volcanic shallow to deeper marine sedimentary rocks lacking thick reef deposits, (iv) post-erosional rejuvenated volcanic rocks, and (v) pelagic sediments. -
Vicente De Gouveia Et Al 2018.Pdf
Earth and Planetary Science Letters 487 (2018) 210–220 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Evidence of hotspot paths below Arabia and the Horn of Africa and consequences on the Red Sea opening ∗ S. Vicente de Gouveia a, , J. Besse a, D. Frizon de Lamotte b, M. Greff-Lefftz a, M. Lescanne c, F. Gueydan d, F. Leparmentier e a Institut de Physique du Globe de Paris - Sorbonne Paris Cité, Université Paris Diderot, UMR CNRS 7154, 1 rue Jussieu, 75252 Paris 05, France b Département Géosciences et Environnement, Université de Cergy-Pontoise, Cergy-Pontoise, France c Total EP, Pau, France d Géosciences Montpellier, Université de Montpellier, CNRS UMR 5243, Montpellier, France e Total EP, Paris La Défense, France a r t i c l e i n f o a b s t r a c t Article history: Rifts are often associated with ancient traces of hotspots, which are supposed to participate to the Received 11 December 2017 weakening of the lithosphere. We investigated the expected past trajectories followed by three hotspots Received in revised form 25 January 2018 (Afar, East-Africa and Lake-Victoria) located around the Red Sea. We used a hotspot reference frame Accepted 29 January 2018 to compute their location with respect to time, which is then compared to mantle tomography Available online xxxx interpretations and geological features. Their tracks are frequently situated under continental crust, which Editor: R. Bendick is known to strongly filter plume activity. We looked for surface markers of their putative ancient Keywords: existence, such as volcanism typology, doming, and heat-flow data from petroleum wells. -
Young Tracks of Hotspots and Current Plate Velocities
Geophys. J. Int. (2002) 150, 321–361 Young tracks of hotspots and current plate velocities Alice E. Gripp1,∗ and Richard G. Gordon2 1Department of Geological Sciences, University of Oregon, Eugene, OR 97401, USA 2Department of Earth Science MS-126, Rice University, Houston, TX 77005, USA. E-mail: [email protected] Accepted 2001 October 5. Received 2001 October 5; in original form 2000 December 20 SUMMARY Plate motions relative to the hotspots over the past 4 to 7 Myr are investigated with a goal of determining the shortest time interval over which reliable volcanic propagation rates and segment trends can be estimated. The rate and trend uncertainties are objectively determined from the dispersion of volcano age and of volcano location and are used to test the mutual consistency of the trends and rates. Ten hotspot data sets are constructed from overlapping time intervals with various durations and starting times. Our preferred hotspot data set, HS3, consists of two volcanic propagation rates and eleven segment trends from four plates. It averages plate motion over the past ≈5.8 Myr, which is almost twice the length of time (3.2 Myr) over which the NUVEL-1A global set of relative plate angular velocities is estimated. HS3-NUVEL1A, our preferred set of angular velocities of 15 plates relative to the hotspots, was constructed from the HS3 data set while constraining the relative plate angular velocities to consistency with NUVEL-1A. No hotspots are in significant relative motion, but the 95 per cent confidence limit on motion is typically ±20 to ±40 km Myr−1 and ranges up to ±145 km Myr−1. -
Sleep, N.H., Hotspots and Mantle Plumes: Some Phenomenology, J
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 95, NO. B5, PAGES 6715-6736, MAY 10, 1990 Hotspotsand Mantle Plumes'Some Phenomenology NORMAN H. SLEEP Departmentsof Geologyand Geophysics,Stanford University, Stanford, California The availabledata, mainly topography, geoid, and heat flow, describinghotspots worldwide are examined to constrainthe mechanismsfor swelluplift and to obtainfluxes and excess temperatures of mantleplumes. Swelluplift is causedmainly by excesstemperatures that move with the lithosphereplate and to a lesser extenthot asthenospherenear the hotspot.The volume,heat, and buoyancy fluxes of hotspotsare computed fromthe cross-sectionalareas of swells,the shapes of nosesof swells,and, for on ridgehotspots, the amount of ascendingmaterial needed to supplythe lengthof ridgeaxis whichhas abnormallyhigh elevationand thickcrust. The buoyancy fluxes range over a factorof 20 withHawaii, 8.7 Mg s -1, thelargest. The buoy- ancyflux for Iceland is 1.4Mg s -1 whichis similarto theflux of CapeVerde. The excess temperature of both on-ridgeand off-ridgehotspots is aroundthe 200øCvalue inferred from petrologybut is not tightly constrainedby geophysicalconsiderations. This observation,the similarityof the fluxesof on-ridgeand off- ridgeplumes, and the tendency for hotspotsto crossthe ridge indicate that similar plumes are likely to cause both typesof hotspots.The buoyancyfluxes of 37 hotspotsare estimated;the globalbuoyancy flux is 50 Mgs -1, whichis equivalentto a globallyaveraged surface heat flow of 4 mWm-2 fromcore sources and wouldcool the core at a rateof 50ø C b.y. -1. Basedon a thermalmodel and the assumption that the likeli- hoodof subductionis independentof age,most of the heatfrom hotspotsis implacedin the lower litho- sphereand later subducted. I.NTRODUCWION ridge plumesusing Iceland as an example. The geometryof flow implied by the assumed existence of a low viscosity Linearseamount chains, such as the Hawaiian Islands, are asthenosphericchannelis illustrated bythis exercise. -
Cretaceous Paleomagnetic Field in North America: True
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 97, NO. B13, PAGES 19,651-19,661, DECEMBER 10, 1992 Paleomagnetismof 122 Ma Plutonsin New England and the Mid-Cretaceous PaleornagneticField in North America' True Polar Wander or Large-Scale Differential Mantle Motion? MICKEY C. VAN FOSSEN AND DENNIS V. KENT Lamont-DohertyGeological Observatory and Departmentof GeologicalSciences, Columbia University, Palisades, iVew York A palcomagneticstudy of CretaceousWhite Mountainsplutonic complexes in New Hampshireand Vermont yields high unblockingtemperature, dual polarity magnetizationsin differenttypes of igneousrocks. The resultingpole position for threeplutons (71.9 ø N, 187.4ø E, A95 = 6.9ø, age= 122.5Ma) agreeswith pre- viously publishedmid-Cretaceous poles for North America, which togethergive a mid-Cretaceousstand- still referencepole slightlyrevised from Globermanand Irving [1988]at 71.2ø N, 194.1ø E (A95 = 3.7ø,N = 5 studies).We argueon the basisof the wide geographicdistribution of thesestudies, the varietyin tec- tonic settingsand rock types,positive reversal tests, and an overall reversalpattern consistent with geo- magneticpolarity time scales,that this mean pole representsthe North Americanmid-Cretaceous reference field for nominally 36 m.y. (124 to 88 Me). The standstillpole limits to within +4 ø, the motion of the North Americanplate relativeto the Earth'sspin axis. During the samemid-Cretaceous interval, the New Englandhotspot track (124 Ma MonteregianHills, 122.5-Ma CretaceousWhite Mountains,and 103- to 84-Me New Englandseamounts) requires 11ø't:4ø of nonh-polewardmotion of North America,in direct conflict with the palcomagneticstandstill. A similar (-13 ø) discrepancyis independentlydemonstrated betweenthe spin axis and the Tristan da Cunha hotspottrack on the African plate during the mid- Cretaceousinterval. •he hotspot/spinaxis discrepanciesended by -90 Ma when it is shownthat both Atlantic hotspotsagree with North Americanand African dipole palcolatitudesand present-daylocations. -
A Plate Model for Jurassic to Recent Intraplate Volcanism in the Pacific Ocean Basin
A Plate Model for Jurassic to Recent Intraplate Volcanism in the Pacific Ocean Basin Alan D. Smith Department of Geological Sciences, University of Durham, Durham, DH1 3LE, UK Email: [email protected] 1 ABSTRACT Reconstruction of the tectonic evolution of the Pacific basin indicates a direct relationship between intraplate volcanism and plate reorganisations, which suggests volcanism was controlled by fracturing and extension of the lithosphere. Middle Jurassic to Early Cretaceous intraplate volcanism included oceanic plateau formation at triple junctions (Shatsky Rise, western Mid Pacific Mountains) and a diffuse pattern of ocean island volcanism (Marcus Wake, Magellan seamounts) reflecting an absence of any well-defined stress field within the plate. The stress field changed in the Early Cretaceous when accretion of the Insular terrane to the North American Cordillera and the Median Tectonic arc to New Zealand, stalled migration of the Pacific- Farallon and Pacific-Phoenix ocean ridges, leading to the generation of the Ontong Java, Manahiki, Hikurangi and Hess Rise oceanic plateaus. Plate reorganisations in the Late Cretaceous resulted from the breakup of the Phoenix and Izanagi plates through collision of the Pacific-Phoenix ocean ridge with the southwest margin of the basin, and development of island arc-marginal basin systems in the northwest of the basin. The Pacific plate nonetheless remained largely bounded by spreading centres, and intraplate volcanism followed pre-existing lines of weakness in the plate fabric (Line Islands), or resulted from fractures generated by ocean ridge subduction beneath island arc systems (Emperor chain). The Pacific plate began to subduct under Asia in the Early Eocene from the record of accreted material along the Japanese margin. -
Hotspot Motion Caused the Hawaiian-Emperor Bend and Llsvps Are Not fixed
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by University of Liverpool Repository ARTICLE https://doi.org/10.1038/s41467-019-11314-6 OPEN Hotspot motion caused the Hawaiian-Emperor Bend and LLSVPs are not fixed Richard K. Bono1,2, John A. Tarduno 1,3 & Hans-Peter Bunge4 Controversy surrounds the fixity of both hotspots and large low shear velocity provinces (LLSVPs). Paleomagnetism, plate-circuit analyses, sediment facies, geodynamic modeling, and geochemistry suggest motion of the Hawaiian plume in Earth’s mantle during formation 1234567890():,; of the Emperor seamounts. Herein, we report new paleomagnetic data from the Hawaiian chain (Midway Atoll) that indicate the Hawaiian plume arrived at its current latitude by 28 Ma. A dramatic decrease in distance between Hawaiian-Emperor and Louisville chain sea- mounts between 63 and 52 Ma confirms a high rate of southward Hawaiian hotspot drift (~47 mm yr−1), and excludes true polar wander as a relevant factor. These findings further indicate that the Hawaiian-Emperor chain bend morphology was caused by hotspot motion, not plate motion. Rapid plume motion was likely produced by ridge-plume interaction and deeper influence of the Pacific LLSVP. When compared to plate circuit predictions, the Midway data suggest ~13 mm yr−1 of African LLSVP motion since the Oligocene. LLSVP upwellings are not fixed, but also wander as they attract plumes and are shaped by deep mantle convection. 1 Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. 2 Geomagnetism Laboratory, University of Liverpool, Liverpool L69 3GP, UK. -
A PLATE TECTONIC RECONSTRUCTION of the SOUTHWEST PACIFIC, 0-100 Ma1
Berger, W.H., Kroenke, L.W., Mayer, L.A., et al., 1993 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 130 43. A PLATE TECTONIC RECONSTRUCTION OF THE SOUTHWEST PACIFIC, 0-100 Ma1 Chun Yeung Yan2 and Loren W. Kroenke3 ABSTRACT Southwest Pacific paleogeography has been reconstructed back to 100 Ma on the basis of the hotspot frame of reference. Plate circuits for all key tectonic elements have been determined with respect to the Indo-Australia (I-A), Antarctica, and Pacific plates, using hotspot trails on the India, Australia, and Pacific plates to constrain the motions of all the plates. Paleo-locations of rifted continental margins, oceanic plateaus, subduction zones, and marginal basins have been reconstructed for the Southwest Pacific in a series of palinspastic maps that are thought to closely portray the tectonic development of the Southwest Pacific during the last 100 m.y. Successive periods of convergence are shown occurring along five different paleo-subduction zones that formed concomitantly with changes in I-A and Pacific plate motions from the Eocene to the late Miocene along the Papuan-Rennell-New Caledonia-Nor- folk (55-40 Ma), Manus-North Solomon-Vitiaz (43-25 Ma), New Guinea-proto-Tonga-Kermadec (27-10 Ma), New Britain-San Cristobal-New Hebrides (12-0 Ma), and Tonga-Kermadec (10-0 Ma) trenches. Episodes of basin formation are shown occurring along the western and southwestern margins of the Pacific Plate and along the eastern and northeastern margins of the I-A Plate from the Late Cretaceous to the present, including the Tasman (85-55 Ma), New Caledonia (74-65 Ma), Coral Sea (63-53 Ma), Loyalty (52-40 Ma), d'Entrecasteaux (34-28 Ma), Caroline (34-27 Ma), Solomon Sea (34-28 Ma), South Fiji (34-27 Ma), North Fiji (10-0 Ma), and Lau, Woodlark, and Manus (5.5-0 Ma) basins. -
Louisville Seamount Trail
IODP Expedition 330: Louisville Seamount Trail Site U1377 Summary Background and Objectives Background Site U1377 (Prospectus Primary Site LOUI-4B) on Hadar Guyot (168.6°W Guyot) was the sixth and last site completed during Integrated Ocean Drilling Program (IODP) Expedition 330. This is also the youngest seamount targeted during Expedition 330 with a measured 40Ar/39Ar age of 50.1 Ma similar to Koko Seamount in the Hawaiian-Emperor Seamount Trail. Hadar Guyot belongs to a cluster of three seamounts that is located in close proximity to the Wishbone Scarp fault zone. Hadar Guyot is the smallest seamount cored during Expedition 330, consisting of a single volcanic center with a base diameter of ~25 km, and like all Louisville seamounts drilled, it has a flat summit plane, defining it as a guyot that at some point must have emerged above sea level as a volcanic island. Site U1377 was placed near the middle of this small edifice, away from its shelf edges and away from any packages of dipping volcaniclastics on its flanks. Sidescan sonar reflectivity survey and 3.5 kHz sub-bottom profiling data indicate that Site U1377 is covered with less than 8 m of pelagic sediment, and seismic reflection profiles show that this site is characterized by a 52 m thick section of dipping volcaniclastics and overlaying igneous basement. The original drilling plan was to recover the soft sediment using a gravity-push approach with little or no rotation using a Rotary Core Barrel (RCB), followed by standard coring into the volcaniclastic material and 350 m into igneous basement.