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1.
Abstract: The bio-essential elements are demanded for the metabolic action of all living organisms. These elements are continuously supplied to biosphere through the elemental cycle on the surface Earth. The geochemical cycle of bio-essential elements was most likely different in the pre-biotic era (ca. 4.4 to 4.0 Ga) compared to the modern Earth. The difference was probably made by the absence of continents and biological mediation in the pre-biotic environments. Geochemical cycle models of bio-essential elements (P, B and Mo) on the pre-biotic Earth are proposed in this study, and these models are examined using available geochemical data.
The input flux of phosphorous in pre-biotic oceans was probably dominated by submarine hydrothermal activities associated with carbonatized oceanic crusts. Such input flux by submarine hydrothermal activities is not known in the present-day oceans, and probably a unique flux in the pre-biotic oceans. Boron chemistry of pre-biotic oceans was also controlled by submarine hydrothermal input flux. The Mo exchange between the pre-biotic ocean and lithosphere may have restricted only at the submarine hydrothermal areas. These suggest that the submarine hydrothermal discharging areas were only locations to obtain bio-essential elements for the earliest life. This model is consistent with the previously proposed model for hydrothermal origin of life. 相似文献
The input flux of phosphorous in pre-biotic oceans was probably dominated by submarine hydrothermal activities associated with carbonatized oceanic crusts. Such input flux by submarine hydrothermal activities is not known in the present-day oceans, and probably a unique flux in the pre-biotic oceans. Boron chemistry of pre-biotic oceans was also controlled by submarine hydrothermal input flux. The Mo exchange between the pre-biotic ocean and lithosphere may have restricted only at the submarine hydrothermal areas. These suggest that the submarine hydrothermal discharging areas were only locations to obtain bio-essential elements for the earliest life. This model is consistent with the previously proposed model for hydrothermal origin of life. 相似文献
2.
Jun Korenaga 《地学学报》2008,20(6):419-439
The chemical composition of the bulk silicate Earth (BSE) indicates that the present‐day thermal budget of Earth is likely to be characterized by a significant excess of surface heat loss over internal heat generation, indicating an important role of secular cooling in Earth’s history. When combined with petrological constraints on the degree of secular cooling, this thermal budget places a tight constraint on permissible heat‐flow scaling for mantle convection, along with implications for the operation of plate tectonics on Earth, the history of mantle plumes and flood basalt magmatism, and the origin and evolution of Earth’s oceans. In the presence of plate tectonics, hotter mantle may have convected more slowly because it generates thicker dehydrated lithosphere, which could slow down subduction. The intervals of globally synchronous orogenies are consistent with the predicted variation of plate velocity for the last 3.6 Gyr. Hotter mantle also produces thicker, buoyant basaltic crust, and the subductability of oceanic lithosphere is a critical factor regarding the emergence of plate tectonics before the Proterozoic. Moreover, sluggish convection in the past is equivalent to reduced secular cooling, thus suggesting a more minor role of mantle plumes in the early Earth. Finally, deeper ocean basins are possible with slower plate motion in the past, and Earth’s oceans in the Archean is suggested to have had about twice as much water as today, and the mantle may have started as dry and have been gradually hydrated by subduction. The global water cycle may thus be dominated by regassing, rather than degassing, pointing towards the impact origin of Earth’s oceans, which is shown to be supported by the revised composition of the BSE. 相似文献
3.
《Chemie der Erde / Geochemistry》2021,81(2):125735
The magma ocean concept was first conceived to explain the geology of the Moon, but hemispherical or global oceans of silicate melt could be a widespread “lava world” phase of rocky planet accretion, and could persist on planets on short-period orbits around other stars. The formation and crystallization of magma oceans could be a defining stage in the assembly of a core, origin of a crust, initiation of tectonics, and formation of an atmosphere. The last decade has seen significant advances in our understanding of this phenomenon through analysis of terrestrial and extraterrestrial samples, planetary missions, and astronomical observations of exoplanets. This review describes the energetic basis of magma oceans and lava worlds and the lava lake analogs available for study on Earth and Io. It provides an overview of evidence for magma oceans throughout the Solar System and considers the factors that control the rocks these magma oceans leave behind. It describes research on theoretical and observed exoplanets that could host extant magma oceans and summarizes efforts to detect and characterize them. It reviews modeling of the evolution of magma oceans as a result of crystallization and evaporation, the interaction with the underlying solid mantle, and the effects of planetary rotation. The review also considers theoretical investigations on the formation of an atmosphere in concert with the magma ocean and in response to irradiation from the host star, and possible end-states. Finally, it describes needs and gaps in our knowledge and points to future opportunities with new planetary missions and space telescopes to identify and better characterize lava worlds around nearby stars. 相似文献
4.
The recent theoretical studies on the formation and evolution of the atmosphere and oceans of the Earth are reviewed. Impact degassing during accretion of the Earth would probably generate an impact-induced steam atmosphere on the proto-Earth. At the end of accretion, the steam atmosphere became unstable and condensed to form the proto-ocean with almost the present mass of ocean. The steam atmosphere would have thus evolved to the proto-CO2 atmosphere during the earliest history of the Earth because CO in the proto-atmosphere may be photochemically converted to CO2. However, CO2 in the proto-atmosphere has decreased with time through the global carbon cycle which may have stabilized the terrestrial environment against an increase in the solar luminosity. The continental growth during Hadean and Archean would therefore have a significant influence on the carbon cycle and the surface temperature. It is also suggested that the continental growth is a necessary condition for the terrestrial environment to evolve to the present state. Both the impact degassing and the subsequent continuous degassing are suggested to have played a major role in the formation and evolution of the atmosphere and ocean. In particular, most of N2 may have been produced by the impact degassing during accretion, and the contribution of the subsequent continuous degassing is at most 10% for N2. As a consequence, after the CO2 level decreased to less than 1 bar, the atmosphere may have been at about 1 bar and composed mainly of N2 for most of the subsequent history of the Earth. 相似文献
5.
Physical state of the very early Earth 总被引：1，自引：0，他引：1
Yutaka Abe 《Lithos》1993,30(3-4):223-235
The earliest surface environment of the Earth is reconstructed in accordance with the planetary formation theory. Formation of an atmosphere is an inevitable consequence of Earth's formation. The atmosphere near the close of accretion is composed of 200 300 bars of H2 and H2O, and several tens of bars of CO and CO2. Either by the blanketing effect of the proto-atmosphere or heating by large planetesimal impacts a magma ocean is formed during accretion. We can distinguish three stages for the thermal evolution of the magma ocean and proto-crust. Stage 0 is characterized by a super-liquidus (or completely molten) regime near the surface. At this stage the surface of the Earth is covered by a super-liquidus magma ocean. No chemical differentiation is expected during this stage. Once the energy flux released by planet formation decreases to the 200 W/m2 level the super-liquidus magma ocean then disappears within a time interval of 1 m.y. This is the transition from stage 0 to 1. Stage 1 is characterized by a partially molten magma ocean. In the magma ocean consisting of 20 30% partial melt, heat transport is controlled by melt-solid separation (a type of compositional convection) rather than thermal convection. Chemical differentiation of the mantle mainly occurs in this stage. Once the energy flux drops to the 160 W/m2 level, more than 90% of water vapor in the proto-atmosphere condense to form the proto-oceans. Several tens of bars of CO and CO2 remain in the atmosphere just after formation of the oceans. Water oceans are occasionally evaporated by large impacts. After each such event, recondensation of the ocean takes several hundred years. Although the surface is covered by a chilled proto-crust, it is short-lived because of extensive volcanic resurfacing activity as well as meteorite impacts resurfacing. This stage ends when the energy flux drops to 0.1 1 W/m2 level. The duration time of stage 1 is estimated to be several hundred million years (the best estimate is about 400 m.y.). Stage 2 is characterized by solid state convection. This stage continues to the present day. One of the most important change on the proto-Earth is the transition from stage 1 to 2, which occurs several hundred million years after the Earth formation. Long-lived crust is formed only after this transition. 相似文献
6.
Bedded sedimentary talc is abundant in Archaean greenstone belts in proximity to seafloor hydrothermal vents. Trace-element abundances and oxygen-isotope evidence suggest formation from heated ocean water. It is suggested that talc forms by reaction of silica in the hot discharge with metal bicarbonate species in ocean water thus releasing carbon dioxide. The possible CO2 flux is similar to the present-day combustion flux and may have maintained a global greenhouse with warm oceans as reflected in the oxygen-isotope systematics of cherts. It seems probable that surface-Earth temperatures may have exceeded the boiling point prior to 4 Ga. If this is possible, then the beginning of the geologic record for the Earth may coincide with the first widespread development of the hydrosphere. 相似文献
7.
海洋N2O的研究进展 总被引：1，自引：0，他引：1
N2O在大气中的浓度仅为CO2的浓度的千分之一左右,但在同等浓度的情况下温室效应却是CO2的200~300倍;它在大气层中的光化学产物会与臭氧反应,从而损耗平流层的臭氧。N2O的环境效应引起人们的关注,许多国际气候变化研究项目都把其列入重要研究内容。通过对过去40年的相关研究工作进行综合分析,阐述N2O在海洋中的分布规律和其影响因素、产生的机制、它的海气通量及其影响因素,从而揭示N2O的海洋生物地球化学循环过程以及这一过程对全球氮循环的贡献。 相似文献
8.
We discuss the potential geodynamic connections between Paleozoic arc development along the flanks of the interior (e.g. the Iapetus and Rheic) oceans and the exterior Paleopacific Ocean. Paleozoic arcs in the Iapetus and Rheic oceanic realms are preserved in the Appalachian–Caledonide and Variscan orogens, and in the Paleopacific Ocean realm they are preserved in the Terra Australis Orogen. Potential geodynamic connections are suggested by paleocontinental reconstructions showing Cambrian–Early Ordovician contraction of the exterior ocean as the interior oceans expanded, and subsequent Paleozoic expansion of the exterior oceans while the interior oceans contracted. Subduction initiated in the eastern segment of Iapetus at ca. 515 Ma and Early to Middle Ordovician orogenesis along the flanks of this ocean is highlighted by arc–continent collisions and ophiolite obductions. Over a similar time interval, subduction and orogenesis took place in the exterior ocean and included formation of the Macquarie arc in the Tasmanides of Eastern Australia and the Famatina arc and correlatives in the periphery of the proto-Andean margin of Gondwana. Major changes in the style of subduction (from retreating to advancing) in interior oceans occurred during the Silurian, following accretion of the peri-Gondwanan terranes and Baltica, and closure of the northeastern segment of Iapetus. During the same time interval, subduction in the Paleopacific Ocean was predominantly in a retreating mode, although intermittent episodes of contraction closed major marginal basins. In addition, however, there were major disturbances in the Earth tectonic systems during the Ordovician, including an unprecedented rise in marine life diversity, as well as significant fluctuations in sea level, atmospheric CO2, and 87Sr/86Sr and 13C in marine strata carbonates. Stable and radiogenic isotopic data provide evidence for the addition of abundant mantle-derived magma, fluids and large mineral deposits that have a significant mantle-derived component. When considered together, the coeval, profound changes in the style of tectonic activity and the disturbances recorded in Earth Systems are consistent with the emergence of a superplume during the Ordovician. We speculate that the emergence of a superplume triggered by slab avalanche events within the Iapetus and Paleopacific oceans was associated with the establishment of a new geoid high within the Paleopacific regime, the closure of the interior Rheic Ocean and the amalgamation of Laurussia and Gondwana, which was a key event in the Late Carboniferous amalgamation of Pangea. 相似文献
9.
M.I. Kuzmin V.V. Yarmolyuk A.B. Kotov N.A. Goryachev 《Russian Geology and Geophysics》2018,59(12):1535-1547
The paper is focused on the evolution of the Earth starting with the planetary accretion and differentiation of the primordial material (similar in composition to CI chondrites) into the core and mantle and the formation of the Moon as a result of the impact of the Earth with a smaller cosmic body. The features of the Hadean eon (ca. 4500–4000 Ma) are described in detail. Frequent meteorite-asteroid bombardments which the Earth experienced in the Hadean could have caused the generation of mafic/ultramafic primary magmas. These magmas also differentiated to produce some granitic magmas, from which zircons crystallized. The repeated meteorite bombardments destroyed the protocrust, which submerged into the mantle to remelt, leaving refractory zircons, indicators of the Early Earth’s geologic conditions, behind.The mantle convection that started in the Archean could possibly be responsible for the Earth’s subsequent endogenous evolution. Long-living deep-seated mantle plumes could have promoted the generation of basalt-komatiitic crust, which, thickening, could have submerged into the mantle as a result of sagduction, where it remelted. Partial melting of the thick crust, leaving eclogite as a residue, could have yielded tonalite-trondhjemite-granodiorite (TTG) melts. TTG rocks are believed to compose the Earth’s protocrust. Banded iron bodies, the only mineral deposits of that time, were produced in the oceans that covered the Earth.This environment, recognized as LID tectonics combined with plume tectonics, probably existed on the Earth prior to the transitional period, which was marked by a series of new geologic processes and led to a modern-style tectonics, involving plate tectonics and plume tectonics mechanisms, by 2 Ga. The transitional period was likely to be initiated at about 3.4 Ga, with the segregation of outer and inner cores, which terminated by 3.1 Ga. Other rocks series (calc-alkaline volcanic and intrusive) rather than TTGs were produced at that time. Beginning from 3.4-3.3 Ga, mineral deposits became more diverse; noble and siderophile metal occurrences were predominant among ore deposits. Carbonatites, hosting rare-metal mineralization, could have formed only by 2.0 Ga. From 3.1 to 2.7 Ga, there was a period of “small-plate” tectonics and first subduction and spreading processes, which resulted in the first supercontinent by 2.7 Ga. Its amalgamation indicates the start of superplume-supercontinent cycles.Between 2.7 and 2.0 Ga, the D″ layer formed at the core-mantle interface. It became a kind of thermal regulator for the ascending already tholeiitic mantle plume magmas. All deep-seated layers of the Earth and large low-velocity shear provinces, called mantle hot fields, partially melted enriched EM-I and EM-II mantles, and the depleted recent asthenosphere mantle, which is parental for midocean-ridge basalts, were finally generated by 2 Ga. Therefore, an interaction of all Earth’s layers began from that time. 相似文献
10.
《Comptes Rendus Geoscience》2018,350(4):154-163
Fluids trapped in inclusions in well-characterized Archaean hydrothermal quartz crystals were analyzed by the extended argon–argon method, which permits the simultaneous measurement of chlorine and potassium concentrations. Argon and nitrogen isotopic compositions of the trapped fluids were also determined by static mass spectrometry. Fluids were extracted by stepwise crushing of quartz samples from North Pole (NW Australia) and Barberton (South Africa) 3.5–3.0-Ga-old greenstone belts. The data indicate that fluids are a mixture of a low salinity end-member, regarded as the Archaean oceanic water, and several hydrothermal end-members rich in Cl, K, N, and radiogenic parentless 40Ar. The low Cl–K end-member suggests that the salinity of the Archaean oceans was comparable to the modern one, and that the potassium content of the Archaean oceans was lower than at present by about 40%. A constant salinity of the oceans through time has important implications for the stabilization of the continental crust and for the habitability of the ancient Earth. 相似文献
11.
V. S. Urusov 《Geology of Ore Deposits》2007,49(7):497-504
A comprehensive statistical analysis of the symmetry of mineral species leads to a definite conclusion that rare minerals possess lower symmetry than abundant ones, so that the most stable minerals are characterized by higher symmetry. Since all recently discovered new minerals belong to rare and very rare species, their percentage is increasing and the mean symmetry index is decreasing with time. In other words, the average symmetry is gradually decreasing with the growing diversity of mineral species. In general, the irreversible process of rare mineral formation obeys the principle of minimum dissymmetrization. At the same time, the reduced symmetry indices strongly decrease on passing from cosmic materials (meteorites, lunar rocks) to the Earth’s solid substances and from the planetary interior (core, mantle) to the Earth’s crust. This trend of the planet’s evolution is related to the pronounced loss of entropy and increase in ordering of solid substances that compose the lithosphere. This is supplemented by the withdrawal of entropy from the solid to the upper liquid (oceans) and gaseous (atmosphere) shells of the Earth and farther to the surrounding space. 相似文献
12.
镁（Mg）作为主要的造岩元素及生物营养元素,是连接大陆、海洋和地球内部循环的重要纽带。碳酸盐岩作为Mg的主要储库,是全球Mg循环的重要组成环节,利用Mg同位素示踪碳酸盐岩沉积—成岩过程是有效反演深时海水Mg同位素组成（δ26Mg海水）、恢复全球Mg循环的基本前提。近二十年来,Mg同位素在示踪碳酸盐岩沉积—成岩过程研究中取得了较大进展:1）不同类型碳酸盐矿物形成过程中的Mg同位素分馏及其影响因素的研究得到完善;2）建立了Mg同位素地球化学模型,对不同白云石化过程进行半定量—定量模拟;3）初步探索了利用Mg同位素反演早期成岩流体体系的方法。以上研究进展为利用碳酸盐岩恢复δ26Mg海水奠定了理论基础,在选择有效的碳酸盐岩载体恢复δ26Mg海水时,需充分考虑碳酸盐岩的沉积—成岩过程及其对Mg同位素组成的影响,并适当结合地球化学模型,消除沉积—成岩因素的影响,进而恢复δ26Mg海水。 相似文献
13.
E.B. Kraus 《Earth》1974,10(3):203-221
Planetary or Rossby waves, though probably unimportant in the fluid interior of the Earth, are of interest to earth scientists in general, because of their pervasive role in the general circulation of oceans and atmospheres. The present review does not presuppose any special knowledge of geophysical fluid dynamics. Following a recapitulation of some general wave concepts, it defines absolute vorticity and its role as a restoring force in rotatory motion. The quasi-geostrophic character, the westward propagation and the dispersion of planetary waves is then discussed, as is the difference between shear waves and waves with vertically uniform motion. A last section deals briefly with the influence of planetary wave dynamics on climatic patterns in the atmosphere and in the oceans. 相似文献
14.
地球和月球起源的非传统模型(英文) 总被引：1，自引：1，他引：0
46亿年以来 ,地球的内力活动是由地球液体内核上升的富氢挥发物流所维持的。为了解释这些导致地球内核如此巨量氢集中的作用 ,文中提出了一个关于地球、其它行星及作为一个整体的太阳系 ,其起源与演化的非传统的岩石学模型。排氢脉冲导致洋壳扩张的增强 ,而此则与创造出造山带的地壳变动幕相关。随后大洋底板活动的减弱 ,则招致褶皱陆壳的剥蚀 ,并伴有广泛展布的玄武岩岩浆作用 ,以及大洋周边优地槽区的稳定化。地壳发展旋回的有规则重复 ,都与地球历史中岩浆作用、变质作用、成矿作用和全球灾变的特殊特点相关。在最大的地核排氢期间 ,氢流体达到了平流层 ,并在这里形成有高反射力的水冰云。它们增加了地球的反射率 ,并成为地球全球冰封的基础。平流层冰云促进了对臭氧辐射盾牌的破坏 ,从而导致继冰期之后的生物灾难。 相似文献
15.
Robert J.Stern 《地学前缘(英文版)》2016,7(4):573-580
As we continue searching for exoplanets,we wonder if life and technological species capable of communicating with us exists on any of them.As geoscientists,we can also wonder how important is the presence or absence of plate tectonics for the evolution of technological species.This essay considers this question,focusing on tectonically active rocky(silicate) planets,like Earth,Venus,and Mars.The development of technological species on Earth provides key insights for understanding evolution on exoplanets,including the likely role that plate tectonics may play.An Earth-sized silicate planet is likely to experience several tectonic styles over its lifetime,as it cools and its lithosphere thickens,strengthens,and becomes denser.These include magma ocean,various styles of stagnant lid,and perhaps plate tectonics.Abundant liquid water favors both life and plate tectonics.Ocean is required for early evolution of diverse single-celled organisms,then colonies of cells which specialized further to form guts,appendages,and sensory organisms up to the complexity of fish(central nervous system,appendages,eyes).Large expanses of dry land also begin in the ocean,today produced above subduction zones in juvenile arcs and by their coalescence to form continents,although it is not clear that plate tectonics was required to create continental crust on Earth.Dry land of continents is required for further evolution of technological species,where modification of appendages for grasping and manipulating,and improvement of eyes and central nervous system could be perfected.These bioassets allowed intelligent creatures to examine the night sky and wonder,the beginning of abstract thinking,including religion and science.Technology arises from the exigencies of daily living such as tool-making,agriculture,clothing,and weapons,but the pace of innovation accelerates once it is allied with science.Finally,the importance of plate tectonics for developing a technological species is examined via a thought experiment using two otherwise identical planets:one with plate tectonics and the other without.A planet with oceans,continents,and plate tectonics maximizes opportunities for speciation and natural selection,whereas a similar planet without plate tectonics provides fewer such opportunities.Plate tectonics exerts environmental pressures that drive evolution without being capable of extinguishing all life.Plate tectonic processes such as the redistribution of continents,growth of mountain ranges,formation of land bridges,and opening and closing of oceans provide a continuous but moderate environmental pressure that stimulates populations to adapt and evolve.Plate tectonics may not be needed in order for life to begin,but evolution of technological species is favored on planets with oceans,continents,plate tectonics,and intermittently clear night sky. 相似文献
16.
The knowledge of Martian salts has gone through substantial changes during the past decades. In the 70th of last century, Viking landers have noticed the existence of salts on Mars. Several salt species have been suggested from then on, such as sulfates and chlorides. However, their origin was a mystery due to the lack of observations. The recent explorations and related studies at the beginning of this century revealed that the crustal composition of Mars is similar to that of Earth, and it was hypothesized that almost one third of Martian surface was covered by oceans and lakes in the early stage of Mars. The huge water bodies may have dissolved a large quantity of ions from Martian primary rocks during the whole Noachian and Hesperian epoch. After the enormous drought event happened during the late Hesperian and the early Amazonian, these dissolved ions have formed huge salts deposits and most of them were preserved on Mars until today. To date, carbonates, sulfates, chlorides have all been detected by orbital remote sensing and by landers and rovers. However, the salt mineral assemblages on Mars seems to have some differences from those on Earth, e.g., rich in sulfates and lack of massive carbonates. To explain this difference, we propose that most of the surface carbonates precipitated from the ancient oceans may have been dissolved by the later ubiquitous acidic fluids originated from the global volcanism in the Hesperian era, and formed the enormous sulfate deposits as detected, and this hypothesis seems to be supported by the evidence that most of the sulfate deposits distribute around the Tharsis volcanic province while the survived carbonates located far from it. This process can release most of the carbon on Mars to the atmosphere in the form of CO2 and then be erased by the late heavy bombardments, which might have profound influence on the climate change happened in the Hesperian age. The positive correlation between the GRS results of the potassium distributions and the distribution of chlorides on Mars, together with the high Br concentration measured from the evaporate sediments at two Mars exploration rover landing sites, indicate that the brines in the regions where the chlorides deposited may have reached the stage for potassium salts deposition, thus we propose for the first time that potassium salts deposits might be prevalent in these regions. 相似文献
17.
N. M. Chumakov 《Stratigraphy and Geological Correlation》2008,16(2):107-119
Ideas of global glaciations on the Earth repeatedly emerged in geology since the middle of the 19th century, but they all did not withstand the test of time. The hypothesis of snowball Earth that suggests long-lasted continuous glaciations over the entire land and oceans in the Late Riphean and Vendian became a popular topic of discussions worldwide. These glaciations must last continuously 15 million years or more owing to enormous stability of climate on the “White Earth,” and one can expect their cessation only when CO2 concentration in the atmosphere is getting by several orders of magnitude higher in the course of volcanic eruptions. However, many sections of the Late Precambrian glacial deposits evidence repeated alternations of glacial and interglacial events of variable rank and oscillations of glaciers. Consequently, liquid water existed on the Earth, hydrological cycle had not been interrupted, and development of phototrophic phytoplankton, the eukaryotic organisms inclusive, was always in progress. These facts and results of the climate mathematical simulation are inconsistent with the concept of long continuous glaciations over the globe and their consequences. Paleomagnetic data represent main starting point of the snowball Earth hypothesis, although they are to a great extent still of insufficient validity for the Precambrian. Equitable criticism of the hypothesis weak sides turns sometimes into denying all the glacial periods of the Late Proterozoic, when tillites are regarded in majority as deposits of subaqueous slumps and debris flows accumulated on walls of oceanic rifts prograding along splitting lines into the Rodinia continent. Doubtless marks of glaciations in the sedimentary succession are regarded therewith as heterochronous indications of local mountain glaciers on risen shoulders of prograding rifts. Widespread occurrence of the Late Precambrian discrete glacial horizons on the platforms means, however, that glaciations of that time have been associated not always with the rifts and consisted of separate glacial events. Glaciogenic horizons comparable in thickness and structure with those of the Phanerozoic Eonothem are also indicative of discrete glacial periods in the Precambrian. Being confined predominantly to the Late Precambrian succession of rifts, these horizons characterize a high burial potential of these structures, whereas outside them glacial horizons of lesser thickness could be easily subjected to erosion. The hypothesis of snowball Earth is inadequately consistent with well-known facts and needs in additional substantiation. There are also grounds to think that oceans have not been completely covered with ice at the time of Precambrian glaciations. 相似文献
18.
CO2 windows from mantle to atmosphere: Models on ultrahigh-temperature metamorphism and speculations on the link with melting of snowball Earth 总被引：8，自引：7，他引：1
We attempt here to correlate the melting phase of major snowball Earth events in the planet with the processes associated with extreme crustal metamorphism and formation of ultrahigh-temperature (UHT) granulite facies rocks. While the dry mineral assemblages that characterize UHT granulites can result from different mechanisms, the direct evidence for the involvement of CO2-rich fluids in generating diagnostic UHT assemblages has been recorded from the common occurrence of pure CO2 fluid inclusions in several terranes. Here we evaluate the tectonic settings under which UHT rocks are generated using modern analogues and show that divergent tectonics—both post-collisional extension and rifting—play a crucial role. In an attempt to speculate the link among CO2 liberation from the carbonated tectosphere, UHT metamorphism and major earth processes, we address some of the important issues such as: (a) how the subcontinental mantle i.e., the tectosphere, had become carbonated; (b) how and when the tectosphere degassed; and (c) what is the difference between Proterozoic orogens and those of the present day. The fate of the Earth as a habitable planet was possibly dictated by a reversal of the fundamental process of formation of oceans through the selective removal of CO2 into mantle in the Hadean times, carbonation of the Archean mantle wedge, and subsequent decarbonation of the carbonated mantle through divergent metamorphism and water infiltration since the Late Proterozoic.The abundant CO2 liberated by subsolidus decarbonation along consuming plate boundaries was probably one of the factors that contributed to the greenhouse effect thereby triggering the deglaciation of snowball Earth. Based on an evaluation of the distribution of carbonated subcontinental mantle in global reconstructions of the Proterozoic supercontinent assembly, and their link with crustal domains that have undergone CO2-aided dry metamorphism at extreme conditions, we speculate that the UHT rocks might represent windows for the transfer of CO2 from the mantle into the mid crust and ultimately to the atmosphere. 相似文献
19.
早新生代是地质史上最后一个温室气候期,随后南极冰盖形成,地球进入到晚新生代冰期。温室气候的成因和冰期气候转型的机制一直是国际相关学界关注的问题。评述国际上对此开展的古气候模拟,反映了早新生代温室气候受到了海洋和大陆的地理位置、暖海洋温盐环流和海洋热输送、太阳辐射和大气CO2浓度变化的作用和影响。古气候模拟还反映了早新生代温室气候转向冰期气候,受到了大洋通道改变和高原构造隆起、大气成分变化以及海陆生态系相互的作用和反馈。这些古气候模拟试验锁定在气候变化的关键时段和重要驱动因子,对测试地球内外驱动力和地球各圈层反馈作用提供了重要的科学依据;温室气候以及趋向冰期气候的模拟研究对探讨气候变化内在机制、预测未来气候具有重要意义。
相似文献
20.
Tectonomagmatic evolution of the Earth and Moon 总被引：1，自引：0，他引：1
The Earth and Moon evolved following a similar scenario. The formation of their protocrusts started with upward crystallization
of global magmatic oceans. As a result of this process, easily fusible components accumulated in the course of fractional
crystallization of melt migrating toward the surface. The protocrusts (granitic in the Earth and anorthositic in the Moon)
are retained in ancient continents. The tectonomagmatic activity at the early stage of planet evolution was related to the
ascent of mantle plume of the first generation composed of mantle material depleted due to the formation of protocrusts. The
regions of extension, rise, and denudation were formed in the Earth above the diffluent heads of such superplumes (Archean
granite-greenstone domains and Paleoproterozoic cratons), whereas granulite belts as regions of compression, subsidence, and
sedimentation arose above descending mantle flows. The situation may be described in terms of plume tectonics. Gentle uplifts
and basins (thalassoids) in lunar continents are probable analogues of these structural elements in the Moon. The period of 2.3–2.0 Ga ago was a turning point in the
tectonomagmatic evolution of the Earth, when geochemically enriched Fe-Ti picrites and basalts typical of Phanerozoic within-plate
magmatism became widespread. The environmental setting on the Earth’s surface changed at that time, as well. Plate tectonics,
currently operating on a global scale, started to develop about ∼2 Ga ago. This turn was related to the origination of thermochemical
mantle plumes of the second generation at the interface of the liquid Fe-Ni core and silicate mantle. A similar turning point
in the lunar evolution probably occurred 4.2–3.9 Ga ago and completed with the formation of large depressions (seas) with thinned crust and vigorous basaltic magmatism. Such a sequence of events suggests that qualitatively new material previously
retained in the planets’ cores was involved in tectonomagmatic processes at the middle stage of planetary evolution. This
implies that the considered bodies initially were heterogeneous and were then heated from above to the bottom by propagation
of a thermal wave accompanied by cooling of outer shells. Going through the depleted mantle, this wave generated thermal superplumes
of the first generation. Cores close to the Fe + FeS eutectics in composition were affected by this wave in the last turn.
The melting of the cores resulted in the appearance of thermochemical superplumes and corresponding irreversible rearrangement
of geotectonic processes. 相似文献