South China Sea) and Their Tectonic Implications
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Seamount Abundances and Abyssal Hill Morphology on the Eastern
GEOPHYSICALRESEARCH LETTERS, VOL. 24, NO. 15,PAGES 1955-1958, AUGUST 1, 1997 Seamountabundances and abyssalhill morphology on the eastern flank of the East Pacific Rise at 14øS IngoGrevemeyer, 12Vincent Renard, 3Claudia Jennrich, • and Wilfried Weigel I Abstract. Bathymetricdata from a Hydrosweepmultibeam hills. Abyssalhills in the PacificOcean form. primarily sonarsurvey of a 720 km longtectonic corridor on theeast througha complexcombination of volcanicconstructional flank of the southernEPR at 14ø14'S coveredabout 25,000 processesand faulting that occur at or nearthe ridgeaxis km2 of zero-ageto 8.5 m.y. old crust(magnetic anomaly [e.g., Golf, 1991; MacdonaMet al., 1996]. Stochastic 4A). In this corridorwe documenta strongcorrelation of analysisof abyssalhills have shownthat ridge flank robustalong flowline changes in abyssalhill morphologyroughness increases with decreasing spreading rate [Menard, and seamountsize distributionwith spreadingrate changes 1967;Malinverno, 199l; Goff, 199l]. Nevertheless,seafloor deducedfrom our magneticdata. Indeed, we find thatboth roughnessvalues show a largevariation along a single rmsheight of abyssalhills andabundance and height of spreadingsegment [Golf, 1991; Goffet al., 1993],suggesting seamountsincrease significantly as spreadingrate changes that spreadingrate cannotbe the solefactor governing from ~ 75 mm/yrto over 85 mm/yr(half rate). Moreover, variationsin abyssalhill morphology. we identified 46 seamountstaller than !.00 m. Previous From November 8 to December 30, 1995 the R/V Sonne studieson the southernEPR reporteda larger densityof carriedout the EXCO-cruise,a geophysicalsurvey on zero- seamounts,organized primarily in chains.Our investigation, age to about8.5 m.y. old seafloor created at the"superfast" however, revealed seamountsnot associatedwith major spreading(full rate >140 mm/yr) East Pacific Rise south of chains,leading us to theconclusion that different forms of the Garrettfracture zone [Weigelet al., 1996]. -
And Post-Collision Calc-Alkaline Magmatism in the Qinling Orogenic Belt, Central China, As Documented by Zircon Ages on Granitoid Rocks
Journal of the Geological Societv. London, Vol. 153, 1996, pp. 409-417. Palaeozoic pre- and post-collision calc-alkaline magmatism in the Qinling orogenic belt, central China, as documented by zircon ages on granitoid rocks F. XUE'.*,',A. KRONER', T. REISCHMANN' & F. LERCH' 'Institut fiir Geowissenschaften, Universitat Mainz, 55099 Mainz, Germany 'Department of Geology, Northwest University, 710069 Xi'an, China .'Present address: Department of Geophysical Sciences, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA Abstract: Basedon large-scale reconnaissance mapping, we identifiedtwo calc-alkaline plutonic assemblagesfrom the northern Qinling orogenic belt.central China. The older assemblage of intrusions. closely associated and deformed coevally with their host volcanic arc sequences, seems to represent the fractionation product of basaltic arc magma. It therefore predates the collision of the North China Block with the Central Qinling island-arc system that developed in a SW Pacific-type oceanic domain south of the North China Block. Single-zircon zo7Pb/2'"Pb evaporation dating yielded early to middle Ordovician ages for this assemblage. with a relatively small range from 487.2 f 1.1 to 470.2 f 1.3 Ma. Intrusions of the younger assemblage are largely undeformed and truncate structures shown in rocks of theolder assemblage. They are interpreted as post-collisional calc-alkaline granitoids.Single zircon dating provided an age of 401.8 f 0.8 Mafor the younger assemblage. consistentwith earlier work that defines an age range from c. 420 to 395Ma. Our datafavour a tectonicmodel involving formation and amalgamation of islandarc and microcontinent terranes between ca. 490 and 470 Ma ago to create the Central Qinling Zone which subsequently collided with theNorth China Block prior to c. -
1 Creating a Species Inventory for a Marine Protected Area: the Missing
Katherine R. Rice NOAA Species Inventory Project Spring 2018 Creating a Species Inventory for a Marine Protected Area: The Missing Piece for Effective Ecosystem-Based Marine Management Katherine R. Rice ABSTRACT Over the past decade, ecosystem-based management has been incorporated into many marine- management administrations as a marine-conservation tool, driven with the objective to predict, evaluate and possibly mitigate the impacts of a warming and acidifying ocean, and a coastline increasingly subject to anthropogenic control. The NOAA Office of National Marine Sanctuaries (ONMS) is one such administration, and was instituted “to serve as the trustee for a network of 13 underwater parks encompassing more than 600,000 square miles of marine and Great Lakes waters from Washington state to the Florida Keys, and from Lake Huron to American Samoa” (NOAA, 2015). The management regimes for nearly all national marine sanctuaries, as well as other marine protected areas, have the goal of managing and maintaining biodiversity within the sanctuary. Yet none of those sanctuaries have an inventory of their known species nor a standardized protocol for measuring or monitoring species biodiversity. Here, I outline the steps required to compile a species inventory for an MPA, but also describe some of stumbling blocks that one might encounter along the way and offer suggestions on how to handle these issues (see Appendix A: Process for Developing the MBNMS Species Inventory (PD-MBNMS)). This project consists of three research objectives: 1. Determining what species inventory efforts exist, how they operate, and their advantages and disadvantages 2. Determining the process of creating a species inventory 3. -
Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets
EPSC Abstracts Vol. 11, EPSC2017-945, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets D. Lourenco, P. J. Tackley, A. Rozel and M. Ballmer Institute of Geophysics, Department of Earth Sciences, ETH Zurich, Switzerland ([email protected] / Fax: +41 44 633 1065) Abstract reported in [3], we use thermo-chemical global mantle convection numerical simulations to Plate tectonics on Earth-like planets is typically systematically investigate the effect of plutonism, in modelling using a strongly temperature-dependent conjugation with eruptive volcanism. Results visco-plastic rheology. Previous analyses have reproduce the three common tectonic/convective generally focussed on purely thermal convection. regimes usually obtained in simulations using a However, we have shown that the influence of visco-plastic rheology: stagnant-lid (a one-plate compositional heterogeneity in the form of planet), episodic (where the lithosphere is unstable continental [1] or oceanic [2] crust can greatly and frequently overturns into the mantle), and influence plate tectonics by making it easier (i.e. it mobile-lid (similar to plate tectonics). At high occurs at a lower yield stress or friction coefficient). intrusion efficiencies, we observe and characterise a Here we present detailed results on this topic, in new additional regime called “plutonic-squishy lid”. particular focussing on the influence of intrusive vs. This regime is characterised by a set of strong plates extrusive magmatism on the tectonic mode. separated by warm and weak regions generated by plutonism. Eclogitic drippings and lithospheric delaminations often occur around these weak regions. -
Volcanism in a Plate Tectonics Perspective
Appendix I Volcanism in a Plate Tectonics Perspective 1 APPENDIX I VOLCANISM IN A PLATE TECTONICS PERSPECTIVE Contributed by Tom Sisson Volcanoes and Earth’s Interior Structure (See Surrounded by Volcanoes and Magma Mash for relevant illustrations and activities.) To understand how volcanoes form, it is necessary to know something about the inner structure and dynamics of the Earth. The speed at which earthquake waves travel indicates that Earth contains a dense core composed chiefly of iron. The inner part of the core is solid metal, but the outer part is melted and can flow. Circulation (movement) of the liquid outer core probably creates Earth’s magnetic field that causes compass needles to point north and helps some animals migrate. The outer core is surrounded by hot, dense rock known as the mantle. Although the mantle is nearly everywhere completely solid, the rock is hot enough that it is soft and pliable. It flows very slowly, at speeds of inches-to-feet each year, in much the same way as solid ice flows in a glacier. Earth’s interior is hot both because of heat left over from its formation 4.56 billion years ago by meteorites crashing together (accreting due to gravity), and because of traces of natural radioactivity in rocks. As radioactive elements break down into other elements, they release heat, which warms the inside of the Earth. The outermost part of the solid Earth is the crust, which is colder and about ten percent less dense than the mantle, both because it has a different chemical composition and because of lower pressures that favor low-density minerals. -
Environmental Effects of Large Igneous Province Magmatism: a Siberian Perspective Benjamin A
20 Environmental effects of large igneous province magmatism: a Siberian perspective benjamin a. black, jean-franc¸ois lamarque, christine shields, linda t. elkins-tanton and jeffrey t. kiehl 20.1 Introduction Even relatively small volcanic eruptions can have significant impacts on global climate. The eruption of El Chichón in 1982 involved only 0.38 km3 of magma (Varekamp et al., 1984); the eruption of Mount Pinatubo in 1993 involved 3–5km3 of magma (Westrich and Gerlach, 1992). Both these eruptions produced statistically significant climate signals lasting months to years. Over Earth’s his- tory, magmatism has occurred on vastly larger scales than those of the Pinatubo and El Chichón eruptions. Super-eruptions often expel thousands of cubic kilo- metres of material; large igneous provinces (LIPs) can encompass millions of cubic kilometres of magma. The environmental impact of such extraordinarily large volcanic events is controversial. In this work, we explore the unique aspects of LIP eruptions (with particular attention to the Siberian Traps), and the significance of these traits for climate and atmospheric chemistry during eruptive episodes. As defined by Bryan and Ernst (2008), LIPs host voluminous (> 100,000 km3) intraplate magmatism where the majority of the magmas are emplaced during short igneous pulses. The close temporal correlation between some LIP eruptions and mass extinction events has been taken as evidence supporting a causal relationship (Courtillot, 1994; Rampino and Stothers, 1988; Wignall, 2001); as geochronological data become increasingly precise, they have continued to indicate that this temporal association may rise above the level of coincidence (Blackburn et al., 2013). Several obstacles obscure the mechanisms that might link LIP magmatism with the degree of global environmental change sufficient to trigger mass extinction. -
Chapter 10: Mantle Melting and the Generation of Basaltic Magma 2 Principal Types of Basalt in the Ocean Basins Tholeiitic Basalt and Alkaline Basalt
Chapter 10: Mantle Melting and the Generation of Basaltic Magma 2 principal types of basalt in the ocean basins Tholeiitic Basalt and Alkaline Basalt Table 10.1 Common petrographic differences between tholeiitic and alkaline basalts Tholeiitic Basalt Alkaline Basalt Usually fine-grained, intergranular Usually fairly coarse, intergranular to ophitic Groundmass No olivine Olivine common Clinopyroxene = augite (plus possibly pigeonite) Titaniferous augite (reddish) Orthopyroxene (hypersthene) common, may rim ol. Orthopyroxene absent No alkali feldspar Interstitial alkali feldspar or feldspathoid may occur Interstitial glass and/or quartz common Interstitial glass rare, and quartz absent Olivine rare, unzoned, and may be partially resorbed Olivine common and zoned Phenocrysts or show reaction rims of orthopyroxene Orthopyroxene uncommon Orthopyroxene absent Early plagioclase common Plagioclase less common, and later in sequence Clinopyroxene is pale brown augite Clinopyroxene is titaniferous augite, reddish rims after Hughes (1982) and McBirney (1993). Each is chemically distinct Evolve via FX as separate series along different paths Tholeiites are generated at mid-ocean ridges Also generated at oceanic islands, subduction zones Alkaline basalts generated at ocean islands Also at subduction zones Sources of mantle material Ophiolites Slabs of oceanic crust and upper mantle Thrust at subduction zones onto edge of continent Dredge samples from oceanic crust Nodules and xenoliths in some basalts Kimberlite xenoliths Diamond-bearing pipes blasted up from the mantle carrying numerous xenoliths from depth Lherzolite is probably fertile unaltered mantle Dunite and harzburgite are refractory residuum after basalt has been extracted by partial melting 15 Tholeiitic basalt 10 5 Figure 10-1 Brown and Mussett, A. E. (1993), The Inaccessible Earth: An Integrated View of Its Lherzolite Structure and Composition. -
And
Sarah Lambart - 2016 Recap Lecture 16: Isotopes 101 • Radioactive (parent) vs. radiogenic (daugher) isotopes • Unstable (radioactive) vs stable isotopes • Uses: for dating (geochronology) and as tracers (source composition) Recap Lecture 16: Isotopes 101 • As tracers: • Ex.: 87Sr/86Sr: DMM < co < cc High Rb/Sr c.c. Crust evolution o.c. 87Sr 86Sr melting event DMM Low Rb/Sr Mantle Primitive Mantle/BSE Depleted mantle evolution € 4.55 b.y. Time -> today Recap Lecture 16: Isotopes 101 • As tracers: • Ex.: 87Sr/86Sr: DMM < co < cc • Isotopes do not fractionate during partial melting and crystallization processes!!! ⇒ 87Sr/86Sr (source) = 87Sr/86Sr (magma) ⇒ if 87Sr/86Sr (magma) ≠ constant ⇒ several source components (subducted oc, subducted sediments, subcontinental lithosphere, ect…) or crustal contamination (AFC) Mid-Ocean Ridges Basalt (MORB) • Facts: • Oceanic floors: 60% of Earth’s surface • Most of the rocks produced at ridges are MORB • Large compositional variability 3) Source composition 2) Melting conditions (Pressure, Temperature) 4) Melt segregation and transport 1) Magma differentiation/crystallization Structure of Mid-Ocean Ridges • Ridges: submarine (most of the time) mountain chains ≈ 3000m Slow-spreading ridge: Fast-spreading ridge: Ex.: Mid-Atltantic ridge : 2cm/yr Ex.: EPR: 10 cm/yr Fig. 13-15 in Winters Structure of Mid-Ocean Ridges • Ridges: submarine (most of the time) mountain chains ≈ 3000m Slow-spreading ridge: Fast-spreading ridge: Ex.: Mid-Atltantic ridge : 2cm/yr Ex.: EPR: 10 cm/yr - Spreading rate: 8-10 cm/yr - Spreading rate: <5 cm/yr - Axial uplift = horst - Axial valley = rift (relief = 300m) - Bigger magma reservoir ⇒ more differentiation - Numerous normal faults: active seismic zone - Small multiple magma reservoirs? The oceanic lithosphere • Maturation d(m) = 2500 + 350 T1/2 (Ma) Fig. -
2019 Annual Report a SUMMARY Climate Change a Triple Threat for the Ocean CO2 Burning Fossil Fuels, Deforestation and Industrial Agriculture Release
2019 Annual Report A SUMMARY Climate Change A triple threat for the ocean CO2 Burning fossil fuels, deforestation and industrial agriculture release carbon dioxide (CO2) and other heat-trapping gases into our atmosphere, causing our planet to warm. The ocean has buffered us from the worst impacts of climate > 90% ~25% HEAT change by absorbing more than 90 CO2 percent of this excess heat and about 25 percent of the CO2, but at the cost of causing significant harm to marine ecosystems. LESS MORE WARMER OXYGEN ACIDIC SEA LEVEL BLEACHING TOXIC ALGAE HABITATS ACIDIFICATION FISHERIES Sea level rise is Warm-water coral reefs Larger and more frequent Lower oxygen levels More acidic water Disruptions in fisheries accelerating, flooding (marine biodiversity blooms are making fish, are suffocating some harms animals that build affect the marine food coastal communities hotspots) could be lost if birds, marine mammals marine animals and shells, such as corals, web, local livelihoods, and and drowning the planet warms by and people sick. shrinking their habitats. clams, and oysters. global food security. wetland habitats. 2°C (3.6°F). In 2019, the Intergovernmental Panel on Climate Change report details the triple threat of climate change to ocean ecosystems: Warming, acidification, and deoxygenation. annualreport.mbari.org/2019 Illustration by Emily Hess Cover photo: Animation by Frame 48 Source: IPCC, 2019: Special Report on the Ocean and Cryosphere in a Changing Climate (SROCC) View from the Masthead Climate Change A triple threat for the ocean CO 2 Advancing science Burning fossil fuels, deforestation and industrial agriculture release and engineering for carbon dioxide (CO2) and other heat-trapping gases into our atmosphere, causing our planet to Earth’s final frontier warm. -
Modeling Seafloor Spreading Adapted from a Lesson Developed by San Lorenzo USD Teachers: Julie Ramirez, Veenu Soni, Marilyn Stewart, and Lawrence Yano (2012)
Teacher Instruction Sheet Modeling Seafloor Spreading Adapted from a lesson developed by San Lorenzo USD Teachers: Julie Ramirez, Veenu Soni, Marilyn Stewart, and Lawrence Yano (2012) Teacher Background The process of seafloor spreading created the seafloor of the oceans. For example, in the Atlantic Ocean, North America and South America moved away from Europe and Africa and the resulting crack was filled by mantle material, which cooled and formed new lithosphere. The process continues today. Molten mantle materials continually rise to fill the cracks formed as the plates move slowly apart from each other. This process creates an underwater mountain chain, known as a mid-ocean ridge, along the zone of newly forming seafloor. Molten rock erupts along a mid-ocean ridge, then cools and freezes to become solid rock. The direction of the magnetic field of the Earth at the time the rock cools is "frozen" in place. This happens because magnetic minerals in the molten rock are free to rotate so that they are aligned with the Earth's magnetic field. After the molten rock cools to a solid rock, these minerals can no longer rotate freely. At irregular intervals, averaging about 200-thousand years, the Earth's magnetic field reverses. The end of a compass needle that today points to the north will instead point to the south after the next reversal. The oceanic plates act as a giant tape recorder, preserving in their magnetic minerals the orientation of the magnetic field present at the time of their creation. Geologists call the current orientation "normal" and the opposite orientation "reversed." USGS Teacher Instruction Sheet In the figure above, two plates are moving apart. -
Provenance and Implication of Carboniferous–Permian Detrital
minerals Article Provenance and Implication of Carboniferous–Permian Detrital Zircons from the Upper Paleozoic, Southern Ordos Basin, China: Evidence from U-Pb Geochronology and Hf Isotopes Ziwen Jiang 1, Jinglan Luo 1,*, Xinshe Liu 2,3, Xinyou Hu 2,3, Shangwei Ma 4, Yundong Hou 2,3, Liyong Fan 2,3 and Yuhua Hu 1 1 State Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Xi’an 710069, China; [email protected] (Z.J.); [email protected] (Y.H.) 2 State Engineering Laboratory of Exploration and Development for Low Permeability Oil and Gas Fields, Xi’an 710018, China; [email protected] (X.L.); [email protected] (X.H.); [email protected] (Y.H.); [email protected] (L.F.) 3 Research Institute of Petroleum Exploration and Development, PetroChina Changqing Oilfield Company, Xi’an 710018, China 4 Shaanxi Mineral Resources and Geological Survey, Xi’an 710068, China; [email protected] * Correspondence: [email protected] Received: 9 February 2020; Accepted: 13 March 2020; Published: 15 March 2020 Abstract: Carboniferous–Permian detrital zircons are recognized in the Upper Paleozoic of the whole Ordos Basin. Previous studies revealed that these Carboniferous–Permian zircons occurred in the Northern Ordos Basin mainly originated from the Yinshan Block. What has not been well documented until now is where this period’s zircons in the Southern Ordos Basin came from, and very little discussion about their provenance. To identify the provenance of the detrital zircons dating from ~350 to 260 Ma, five sandstone samples from the Shan 1 Member of Shanxi Formation and eight sandstone samples from the He 8 Member of Shihezi Formation were analyzed for detrital zircon U-Pb age dating and in situ Lu-Hf isotopic compositions. -
Publications Supported by NOAA's Office of Ocean Exploration And
1 Publications Supported by NOAA’s Office of Ocean Exploration and Research Compiled by Chris Belter, NOAA Central Library Accurate as of 17 April 2012 Journal Articles (n=454) Ahyong ST. 2008. Deepwater crabs from seamounts and chemosynthetic habitats off eastern New Zealand (Crustacea : Decapoda : Brachyura). Zootaxa(1708):1-72. Aig D, Haywood K. 2008. Through the Sea Snow: The Central Role of Videography in the Deep Gulf Wrecks Mission. International Journal of Historical Archaeology 12(2):133-145. doi:10.1007/s10761-008-0049-7 Andrews AH, Stone RP, Lundstrom CC, DeVogelaere AP. 2009. Growth rate and age determination of bamboo corals from the northeastern Pacific Ocean using refined Pb-210 dating. Marine Ecology-Progress Series 397:173-185. doi:10.3354/meps08193 Angel MV. 2010. Towards a full inventory of planktonic Ostracoda (Crustacea) for the subtropical Northwestern Atlantic Ocean. Deep-Sea Research Part Ii-Topical Studies in Oceanography 57(24-26):2173-2188. doi:10.1016/j.dsr2.2010.09.020 Arellano SM, Young CM. 2009. Spawning, Development, and the Duration of Larval Life in a Deep-Sea Cold-Seep Mussel. Biological Bulletin 216(2):149-162. Auster PJ. 2007. Linking deep-water corals and fish populations. Bulletin of Marine Science 81:93-99. Auster PJ, Gjerde K, Heupel E, Watling L, Grehan A, Rogers AD. 2011. Definition and detection of vulnerable marine ecosystems on the high seas: problems with the "move-on" rule. ICES Journal of Marine Science 68(2):254-264. doi:10.1093/icesjms/fsq074 Auster PJ, Watling L. 2010. Beaked whale foraging areas inferred by gouges in the seafloor.