Influence of hydrodynamic regime on the mineral composition of deep-sea sediments

The composition of sand-silt and pelite fractions of deep-sea sediments deposited under different hydrodynamic conditions was studied. Assemblages of clastic, clayey, biogenic, and authigenic minerals formed under the influence of surface and bottom currents were traced. It is shown that biogenic opal, fine-dispersed celestobarite, and authigenic protosyngenetic ferromanganese micronodules, which are composed of only manganese phases, represent indicators of cyclonic gyres characterized by enhanced bioproductivity. Collophane (bone detritus), phillipsite, palagonite, and large celestobarite crystals prevail in mineral assemblages below the anticyclonic gyres, whereas ore micronodules are depleted in manganese. Surface and bottom currents control the distribution of clastic (terrigenous edaphogenic, terrestrial-volcanogenic) and clay minerals, as well as biogenic opal in the form of Ethmodiscus frustules in sediments. Edaphogenic mineral assemblages represent the reliable indicators of bottom currents.     

Iodine diagenesis in non-pelagic deep-sea sediments

Measurements of sediment geochemistry and porewater speciation have been made using eight cores containing turbidite sections from the Madeira and Nares Abyssal Plains. The results have been used to evaluate how the diagenetic chemistry of iodine in these sediments compares with that in sediments undergoing steady-state diagenesis. The behaviour of iodine is related to the development of a redox front within the turbidite, between the organic-rich anoxic sediment and its oxic cap, and the downward migration of the front through the turbidite with time. In contrast to the steady-state case, sediment I contents and I/ C ratios increase downwards through the oxidised section reaching a maximum at the redox front (up to ~ 100 μ/g I; molar I/C~ 20 × 10⁻⁴) below which values drop dramatically (I/C ~ 5 × 10⁻⁴). A strong iodate enrichment (up to ~3 μmol kg⁻¹) is observed in the oxidised section of the sediment. At the front interconversion of I⁻ and IO⁻₃ species occur and below the front porewater IO⁻₃ is absent and I~ concentrations increase with depth (as in other cases of anoxic diagenesis) up to ~ 10 μmol kg⁻. In the oxidised section of the sediment the I enrichment has been supplied by upward transport of iodide with the increasing I content, with depth being accounted for by progressive diagenetic enrichment with time.     

Iodine diagenesis in pelagic deep-sea sediments

Nineteen sediment cores from the Madeira, Seine, Tagus and Nares Abyssal Plains and the Alboran Sea have been used to evaluate the speciation, fluxes and diagenesis of iodine in the deep sea. The sediments have surficial molar I/C ratios of 10–30 × 10⁻⁴ in excess of previous reported values for planktonic material (~1 × 10⁻⁴). Solid phase I contents decrease exponentially with depth corresponding to decomposition rate constants of 5–260 × 10⁻⁶ yr⁻¹ which vary with the carbon accumulation rate.Iodine species in the pore waters follow a vertical sequence of four zones: 1. a zone of I⁻ production where total dissolved iodine (∑I) concentrations initially increase at the seawater-sediment interface; 2. a zone of I⁻ oxidation where interconversion of I⁻ to IO⁻₃ occurs; 3. a zone of IO⁻₃ reduction where interconversion of IO⁻₃ back to I⁻ occurs which corresponds to the suboxic part of the sediment column; and 4. a further zone of I⁻ production which is confined to the lower anoxic part of the sediment column. Benthic ∑I fluxes in the Madeira Abyssal Plain measured from shipboard incubation experiments and calculated from porewater gradients are similar, averaging 0.55 and 0.36 × 10⁻⁸ μmol cm⁻² sec⁻, respectively.In the surface sediment the observed I enrichment results from a quasi-closed cycle for iodine initially involving release of I⁻ from decomposing marine organic matter followed by rapid removal onto organic matter at the sediment-seawater interface where I/C regeneration ratios of up to 200 × 10⁻⁴ are found, lodate reduction occurs during suboxic diagenesis, after denitrification and before MnO₂ reduction, consistent with the sequence of reactions predicted from the free energy yields for organic matter oxidation. There is some further I⁻ production in the anoxic section of sediments but at much smaller rates than occur during the interfacial diagenetic cycling.     

Uranium in pacific deep-sea sediments and manganese nodules

A total of 1344 manganese nodules and 187 pelagic sediments from 9 areas in the North and the South Pacific were analyzed for U by the delayed-neutron counting technique. A strong positive correlation between U and Fe in nodules and sediments suggests a co-precipitative removal from sea water into the Fe-rich ferromanganese mineral phase δ -MnO₂. Enrichment of U and Fe in nodules from the northwestern slopes of two submarine hills (U between 6 and 9 ppm) in the equatorial nodule belt is thought to be caused by directional bottom water flow creating elevated oxygenized conditions in areas opposed to the flow. Economically important nodule deposits from the nodule belt and the Peru Basin have generally low U contents, between 3 and 5 ppm. Insignificant resources of U of about 4 × 10⁵ in the Pacific manganese nodules are estimated.     

Diffusion of ions in sea water and in deep-sea sediments

The tracer-diffusion coefficient of ions in water, D_j⁰, and in sea water, $\text{D}{}_{\mathrm{j}}{}^1$, differ by no more than zero to 8 per cent. When sea water diffuses into a dilute solution of water, in order to maintain the electro-neutrality, the average diffusion coefficients of major cations become greater but of major anions smaller than their respective $\text{D}{}_{\mathrm{j}}{}^1$ or D_j⁰ values. The tracer diffusion coefficients of ions in deep-sea sediments, D_j,sed., can be related to $\text{D}{}_{\mathrm{j}}{}^1$ by $\text{D}{}_{\mathrm{j,sed.}}\text{= D}{}_{\mathrm{j}}{}^1\text{·}\text{α}\text{θ}{}^2$, where θ is the tortuosity of the bulk sediment and a a constant close to one.     

26Al-10Be systematics in deep-sea sediments

We report the development of a NaOH-leaching technique to extract the authigenic Al and Be in marine sediments, which should allow the sedimentary signals of cosmogenic ²⁶Al and ¹⁰Be to be more effectively studied as geochemical/geophysical tracers. The technique has been applied to the study of ²⁶Al and ¹⁰Be in opal-rich sediments from the North Pacific. The ²⁶Al/²⁷Al and ¹⁰Be/⁹Be ratios of ~3 × 10⁻¹⁴ and 1 × 10⁻⁷ leached from the sediments are higher than those in the total sediments by factors of 3–10 and 2–3, respectively. The authigenic ¹⁰Be/⁹Be ratios are similar to those in deep waters at the study site, pointing to the potential usefulness of the ratios in paleoceanographic studies. The fractions of total Be and Al in the sediment studied that are of authigenic origin average about 40 and 17%, respectively. Estimated ²⁶AL/²⁷A1 ratios in detrital sediments are ≤ 10⁻¹⁵, low enough to indicate that the source of ²⁶Al in the ocean mainly comes from atmospheric production. In the study area, the deposition flux of ²⁶Al is comparable to its atmospheric supply. However, the deposition flux of ¹⁰Be is about threefold higher than the atmospheric input, signifying lateral transport of ¹⁰Be from the open ocean to this area of relatively high particle flux. The ²⁶Al/¹⁰Be ratio, being insensitive to the oceanic influx of lithogenic particles, may serve as a valuable proxy for paleoproductivity. Both the authigenic and total-sediment ²⁶Al/²⁷Al and ¹⁰Be/ ⁹Be ratios decreased significantly at ~6 ka, which could reflect an enhanced input of windblown lithogenic particles to the North Pacific. While the enhanced dust input did not significantly alter the deep-water ⁹Be concentration, it contributed to the observed increase of authigenic ⁹Be flux to the sediment.     

Formation and reactions of alkyl adamantanes in sediments: Carbon surface reactions

Diamondoids are hydrocarbons with a carbon skeleton that is superimposable on the diamond lattice. Adamantane is the cage-shaped primary unit of diamondoids and occurs widely in sediments and petroleum. The first report of adamantane isolated from petroleum extends back seven decades, but the precursors and reaction mechanisms for the formation of adamantane and related diamondoids in sediments has remained unclear. We report the formation of alkyl adamantanes by heating β-ionone with activated carbon in closed system pyrolysis experiments in the range 170-320 °C. In addition, hydrogen exchange, demethylation, methyl transfer and isomerisation reactions were observed when the model compounds adamantane and 1,3-dimethyladamantane were heated at moderate temperature with activated carbon. A reaction pathway for the formation and reactions of alkyl adamantanes is proposed on the basis of ring isomerisation of adamantane to protoadamantane on the activated carbon surface. The carbonaceous surface reactions described help account for the occurrence and distribution of alkyl adamantanes in petroleum basins, as evidenced by the strong linear relationships between compound pairs related by isomerisation and demethylation for a set of crude oils from the Carnarvon Basin, Western Australia.     

Micromanganese nodules in deep-sea sediments: Uranium-isotopic evidence for post-depositional origin

Micromanganese nodules from three deep-sea cores are found to contain less U than average nodules dredged from the sea floor. The ${}^{234}\text{U}{}^{238}\text{U}$ ratio in these micronodules is higher than any previously reported in deep-sea sediments. We interpret these data to mean that at least some micronodules form well after deposition of the enclosing sediments, in particular where conditions are less oxidizing than average.     

深海沉积物中的稀土矿产资源研究进展

近年发现,太平洋和印度洋的深海盆地中存在大量富含稀土的深海沉积物。主要类型为多金属软泥、沸石黏土和远洋黏土,其中的全稀土含量(∑REY,∑REE+Y)为400×10-6~2000×10-6,最高可达6600×10-6,重稀土含量(HREE)已达到或超过中国南方离子吸附型矿床的重稀土品位两倍以上,是潜在的新型稀土资源,具有重要的经济价值。目前不少学者对富稀土的深海沉积物进行了大量地球化学及部分矿物学的工作,认为多金属软泥中的稀土元素多赋存于与海底热液作用有关的铁锰氧化物和氢氧化物中,而沸石黏土和远洋黏土中稀土元素的富集则与磷酸盐的混入密切相关,其稀土元素主要存在于与磷灰石成分相当的生物鱼骨屑中。深海黏土的北美页岩标准化稀土配分模式与海水相似,表明其中的稀土元素主要来自于海水,REY富集成矿可能主要受控于磷灰石早期成岩阶段,期间稀土元素未发生分异。尽管近些年对深海沉积物中的稀土元素研究取得了不少成果,但是,对于沉积物中的稀土富集机制及影响因素等问题仍然需要更加深入的研究。作为稀土资源大国,为了争取我国在国际海底稀土资源竞争中的话语权,维护中国的稀土利益,中国应加紧开展相关的稀土资源勘查和潜力评价。     

Sources for gold,palladium and iridium in deep-sea sediments

Deep-sea sediment cores, one from the Caribbean (calcareous ooze) and three from the Pacific-Antarctic basin (Globigerina ooze, siliceous ooze and pelagic clay) were analysed for Au, Pd, Ir and Mn by neutron activation. The average noble metal contents for 37 samples are: Au (ppb) Pd (ppb) Ir (ppb) 1.05 ± 0.9 3.5 ± 2.8 0.31 ± 0.14 Biogenic and lithogenic (terrigenous) constituents account for much of the noble metal in these sediments. The average noble metal content, particularly that of Au and Ir, shows little variation over the entire suite of four cores despite large differences in the proportions of biogenic and lithogenic fractions. In general neither component is a markedly more significant noble metal sink than the other. However, a strong correlation between Au and CaCO₃ in the Caribbean calcareous ooze suggests that the biogenic fraction is a significant concentrator in this core.Palladium content is more variable than that of Au or Ir and in two of the Antarctic cores some Pd, probably of hydrogenous origin, is present.The Ir content of all cores is higher than that expected of purely terrigenous sources and there is little suggestion of biogenic concentration of the metal. $\text{Au}\text{Ir}$ ratios differ greatly from average continental crust but are similar to oceanic crust. In one of the Antarctic cores some Ir of hydrogenous and of extraterrestrial origin may be present.     

Implications of precise 10Be measurements in deep-sea sediments

Precise ¹⁰Be measurements in a vertical profile of a large-diameter gravity core with uniform chemical composition from the central equatorial Pacific have not shown the expected decrease with depth. The decay-corrected ¹⁰Be activities ranged from 5.79 ± 0.21 d.p.m. kg^?1 at the top of the core to 9.88 ± 0.46 d.p.m. kg^?1 at the bottom, with a mean of 7.24 ± 1.18 d.p.m. kg^?1. This variation is attributable to the combined variations in the intensity of cosmic rays and that of the earth's magnetic field during the past ～ 1 Ma.     

Straightchain geolipids of deep-sea sediments: Comparison of two extraction procedures

The effects of carbonate demineralization with acid upon geolipid extraction yields were assessed in samples of Pleistocene and Miocene deep-sea sediments. Distributions of free and bound geolipids were similar in extracts from demineralized and intact sediment. Although amounts of n-alkanes were not affected, n-alkanoic acids and n-alkanols experienced losses as a result of demineralization. The biogenic carbonates in these old but nonlithified sediments evidently harbor low concentrations of lipid material, and demineralization of sediments is not recommended for routine use without prior testing.     

深海沉积物与履带相互作用试验研究

深海沉积物与履带相互作用的力学特性是深海资源采运设备设计的重要依据。在国内外专家调查、研究的基础上,以膨润土与水的混合物代替深海沉积物,将履带分解为压陷板和剪切板,在特制的试验槽内开展了沉积物的压力沉陷试验与剪切变形试验,得到了沉积物与履带相互作用的压力-沉陷关系曲线和剪应力-剪切位移关系曲线。基于Bekker沉陷模型,得到了模拟沉积物压力-沉陷模型的各个参数值;同时,发现模拟沉积物剪切变形过程具有明显的阶段性,具体可分为线弹性阶段、应变强化阶段、应变软化阶段和残余应力阶段     

A unified approach to mechanical compaction,pressure solution,mineral reactions and the temperature distribution in hydrocarbon basins

In modelling sediment compaction and mineral reactions, the rheological behaviour of sediments is typically considered as poroelastic or purely viscous. In fact, compaction due to pressure solution and mechanical processes in porous media is far more complicated. A generalised model of viscoelastic compaction and the smectite to illite mineral reaction in hydrocarbon basins is presented. A one-step dehydration model of the mineral reaction is assumed. The obtained non-linear governing equations are solved numerically and different combinations of physical parameters are used to simulate realistic situations in typical sedimentary basins. Comparison of numerical simulations with real data has shown very good agreement with respect to both the porosity profile and the mineral reaction.     

Position of zone of reverse magnetic polarity in deep-sea sediments

We consider the tectonic structure of the eastern part of the Chukotka fold belt, classify the magmatic formations by types of intrusions, and record the basic patterns in distribution of gold and tin-tungsten mineralization. Three structures have been recognized: the Chaun-Iul'tin and Vankarem anticlinal zones and the Amgueroa synclinal zone, complicated by block and linear-folded structures of higher orders.

The magmatic formations consist of Early Triassic gabbros, pre-batholithic dikes, and small bodies of diorites, granodiorites, and lamprophyres. Late Jurassic-Early Cretaceous granitoid batholith-like massifs of the Metegyn- Veshkap type. Early Cretaceous granitoid bodies of the Iul'tin, and Late Cretaceous jointed granitoid massifs of the Telekay type

Gold within the anticlinal zones displays an association with the batholith-like massifs of the Metegyn-Veshkap type and with the pre-batholithic dikes of intermediate composition. In the Amguema zone, the sources of the gold were apparently intrusive bodies of intermediate composition, associated with the formation of the Ohkotsk-Chukotka volcanic belt. Tin and tin-tungsten deposits of the cassiterite-quartz association, distributed within the anticlinal zones, display an association with granites of the Iul'tin type; tin deposits of the cassiterite-silicate association concentrate mainly toward the Amguema synclinal zone and are associated with granites of the Telekay type. —Authors.     

Modeling reactive transport in sediments subject to bioturbation and compaction

Current bioturbation models are marked by confusion in their treatment of porosity. Different equations appear to be needed for different biodiffusion mechanisms, i.e., interphase mixing, where biological activity causes bulk mixing of sediment affecting both tracer and porosity profiles, versus intraphase mixing, where the solid components are intermixed, but the porosity is left unchanged. Another issue is whether the model depends upon the particle type with which tracers are associated, e.g., ¹³⁷Cs on small clay particles versus ²¹⁰Pb on larger grains. This uncertainty has lead to conflicting conservation equations for radiotracers, and in particular, to the question whether the porosity should be placed inside or outside of the differential term that governs the biodiffusive flux. We have reexamined this situation in the context of multiphase, multicomponent continuum theory. Most importantly, we prove that under the assumption of steady-state porosity, there exists only one correct form of the steady-state conservation equation for a radiotracer, regardless of biodiffusion mechanism and particle type, i.e.,

     

On the relationship between silica and carbonate diagenesis in deep-sea sediments

Silica diagenesis and carbonate diagenesis are interrelated. This is confirmed by observations of DSDP Sites 462, 463, 465, 466, and 577. Carbonate sediments containing chert (1) tend to be more indurated and display more advanced diagenetic alterations, regardless of sub-bottom depth; and (2) microfossil components are more strongly affected (overgrown and/or dissolved), while the amount of micritic particles and larger, euhedral calcite crystals is greater. In addition, mass physical properties, porosity in particular, vary more widely in sediment sections containing chert. Furthermore, in the studied similarly composed sediments recrystallization of biogenic opal is indicated by a significant reduction of the specific surface area, reaching a minimum value when quartz is formed.One possible mechanism involved is the production of «surplus« dissolved carbonate created by the replacement of carbonate material by silica during the process of chert formation and silicification. The «extra« carbonate is then available for precipitation as overgrowths and cement outside the chert nodules and silicified zones. Hence silica diagenesis, if it occurs early enough in the sediment, bears some influence on carbonate diagenesis. It is therefore suggested that silica diagenesis be added to the list of factors included in the «diagenetic potential« equation ofSchlanger &Douglas (1974).

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Zusammenfassung Die Diagenese von biogenem Silikat und Karbonat steht in engem Zusammenhang, wie Beobachtungen an Sedimenten der DSDP Sites 462, 463, 465, 466 und 577 zeigen. Karbonatische Sedimente, die biogenes SiO₂ enthalten, zeichnen sich aus durch (1) größere Verfestigung und stärkere diagenetische Veränderungen — unabhängig von der Tiefe im Sediment, (2) mehr Lösung und Überwuchs an Mikrofossil-Komponenten, (3) höheren Anteil mikritischer Partikel wie auch größerer idiomorpher Kalzitkristalle, (4) stärkere Variation der sedimentphysikalischen Eigenschaften, speziell der Porosität und damit zusammenhängender Parameter.Die Umkristallisation des biogenen SiO₂ führt in ähnlich Zusammengesetzen Sedimenten zu einer drastischen Abnahme der spezifischen Oberfläche. Minimalwerte werden erreicht, wenn sich Quarz bildet.Diagenetisch wichtig ist die Produktion von zusätzlichem Karbonat durch die Silizifizierung von Karbonatschalen. Dieses »Überschuß«-Karbonat wird dann als Überwuchs, Zement oder außen an den »Hornstein«-Aggregaten gefällt. Demzufolge beeinflußt die Diagenese von biogenem SiO₂ auch die Karbonatdiagenese. Daher ist es sinnvoll, die Diagenese von biogenem SiO₂ mit zu den Faktoren zu rechnen, die das »diagenetische Potential« — wie esSchlanger &Douglas (1974) definierten — ausmachen.

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Résumé L'étude de sédiments provenant des sites DSDP 462, 463, 465, 466 et 577 montre qu'il existe une relation entre la diagenèse de la silice et celle du carbonate biogéniques. Les sédiments carbonatés qui renferment de la silice biogémque présentent: 1) une induration plus marquée et des modifications diagénétiques plus poussées — et ce indépendamment de la profondeur sous la surface du fond; 2) une dissolution et/ou un accroissement plus développés des micro-fossiles; 3) une plus grande teneur en particules micritiques et une plus grande taille des calcites idiomorphes; 4) un éventail plus large de leurs propriétés physiques, particulièrement de la porosité et des paramètres qui en dépendent.La cristallisation de l'opale biogénique, dans des sédiments de compositions semblables, se traduit par une réduction drastique de la surface spécifique, qui atteint une valeur minimale lorsque du quartz est formé.Un rôle diagénétique important est joué par l'excès de carbonate dissous engendré par la silicification de coquilles carbonatées; cet excès de carbonate est dès lors disponible pour la précipitation des auréoles d'accroissement et du ciment hors des nodules de chert et des zones silicifiées. Il s'ensuit que la diagenèse du SiO₂ biogénique influence la diagenèse du carbonate. Il conviendrait dès lors d'ajouter la diagenèse de la silice à la liste des facteurs qui interviennent dans l'équation du «potentiel diagénétique» deSchlanger etDouglas (1974).

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462, 463, 465, 466 577, . , , : 1) , ; 2) ; 3) , 4) , . SiO₂ . . . »« , , « ». , .. «, 1974 Schlanger & Douglas.

     

Modelling of porosity evolution and mechanical compaction of calcareous sediments

A continuum mechanics model for the gravitational compaction of sediments is derived by assuming that the sediments are normally pressured and in a one-dimensional state of stress. Sediment strength is characterized in terms of effective stress laws adopted from soil mechanics. The model is a relatively simple mathematical formula that gives the porosity as a function of burial depth. The shape of the porosity profile is controlled by two mechanical parameters, the compression index and the void ratio at an effective stress of 100 kPa. The model was verified by analysing the porosity—depth data of oozes and chalk from the Ontong Java Plateau, gathered during Leg 130 of the Ocean Drilling Program. The mechanical parameters of the sediments were estimated using a least-squares method to fit the theoretical profile to the porosity data. The theoretical profile described accurately the ooze porosity data over depth ranges of 100 m or more. However, over smaller length-scales of 10–50 m there were systematic deviations between the theoretical porosity values and the ooze porosity data. The porosity deviations correlated with variations in the mean grain size of the sediments, due in part to changes in the foraminifera abundance. In the case of the oozes, the estimated mechanical parameters were consistent with published values obtained from one-dimensional compression tests. In contrast, the estimated mechanical properties for the chalks differed from published values. The chalk porosities were lower than could be explained by mechanical compaction. This explanation is supported by the compressional (P-wave) velocity data. In the chalk sections, the P-wave velocity increases more rapidly with burial depth than it does in the ooze sections, suggesting that sediment elastic properties are increasing due to interparticle binding.     

Diterpenoid compounds and other lipids in deep-sea sediments and their geochemical significance

Cyclic diterpenoid compounds have been found by various investigators in the geosphere (e.g. fossil resins, coals, soil, shale and deep-sea sediments). These compounds occur in significant amounts only in higher plants and are therefore potential markers of terrigenous plant lipids.Diterpenoids with the abietane skeleton (mainly dehydroabietic acid) have been identified in the lipids of sediment samples from the northeast Pacific Ocean, Black Sea and North Atlantic Ocean. The presence of these resin-derived compounds correlated with the terrigenous clay components and with the presence of pollen. The presence of polycyclic diterpenoids was also correlated with the distribution patterns and inferred sources of other sediment lipid constituents (e.g. n-alkanes, n-fatty acids, etc.).Potamic transport, followed by turbidite redistribution are the probable input mechanisms of these resin-derived compounds to the deep-sea sediments. These diterpenoids appear to be excellent biological markers of resinous higher plants.     

A normative calculation technique for determining opal in deep-sea sediments

The opal content of deep-sea sediment can be estimated by subtracting non-biogenic silica, calculated from the aluminum and magnesium concentrations in the sediment, from the total silica content of the samples. Unlike most previously described methods, this calculation is capable of yielding reliable estimates of opal in pre-Pleistocene sediments because it is unaffected by structural changes that take place in opal as it ages.