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1.
万天丰 《地学前缘》2018,25(2):320-335
全球板块构造的动力学机制问题是一个热门但至今尚未解决的难题。本文首先回顾了近百年来大地构造学的各种主要假说和近四十年来板块构造学说的许多新进展。在上述研究的基础上, 受Rampino和Stothers关于陨击作用可引起地表重大灾变事件思想的启发,笔者提出了一个新的假说。基于中、新生代(200 Ma以来)每隔33 Ma太阳系就会穿越一次银河系星际物质密集的银道面,诱发太阳系内部引力场的巨变,使部分小行星失稳,从而撞击地球。笔者根据用以描述中生代以来全球板块构造的七种不同的运动模式, 提出了巨大陨星在不同地点、以不同角度撞击地表岩石圈,可能诱发地幔底辟的形成,从而推动板块呈放射状或单向运移的假说,也即在200、170、100、65和0.78 Ma等时期的陨击事件基本上是垂直地表面而撞击的,从而诱发地幔底辟的形成和岩石圈板块的放射状张裂和运移;138 Ma的陨击事件可能是指向印度板块的斜向撞击;而35 Ma时期的微玻璃陨石撞击事件则是陨石以极低角度撞击地球表面的表现。陨石撞击地球,这是太阳系内部各星体之间引力作用变化的表现,因而此假说不是什么外因作用论。  相似文献   

2.
陨星撞击地球将是21世纪的研究热门   总被引:5,自引:0,他引:5  
人类对陨星撞击的研究,始于1609年,当时伽利略凭望远镜对月球表面环形“斑点”的观察,提出月坑陨击成因的科学见解。1906年,D.M.巴林格成功地论证了地球上第一个陨星撞击构造——美国亚里桑那州梅蒂尔(Meteor)陨击坑。嗣后,据原苏联和美国宇宙飞行探测所取得的丰富资料,特别是1969年人类首次踏足月球以来,认为陨星撞击作用是太阳系各星球上已知最基本的“地质”作用,所有星球都遭受过陨星的撞击,地球也绝不例外。从此在地球上  相似文献   

3.
寒武纪早期大气-海洋氧含量与生命大爆发   总被引:1,自引:0,他引:1  
寒武纪早期(541~510Ma)地球环境与这一时期生命大爆发之间的关系一直是地球生物学研究的热点问题之一。本文系统总结了目前寒武纪早期大气-海洋氧含量与这一时期生命辐射之间关系的3种假说:大气-海洋的氧含量增加导致了寒武纪生命大爆发;寒武纪生命大爆发导致了大气-海洋氧化以及二者之间没有因果关系。3种假说均有相应的支持证据,但也存在与寒武纪早期海洋化学记录、与现代海洋观察不符和上述假说均未考虑寒武纪早期生命演化所展示的时空差异性等问题。在上述3种假说的基础之上,本文通过对寒武纪构造活动、陆源输入、海洋化学和生命演化等最新资料的综合讨论和分析表明:寒武纪早期地球环境与生命辐射之间很可能是相互作用与协同演化关系,而非简单的单向关系。  相似文献   

4.
一、前寒武纪地层学和古生物学研究的重要性目前,一般认为地球的年龄是47-45亿年,最早的地质旋回开始的时间是40亿年,而地质历史和生物发展发生根本变化的寒武纪下限是5.7-5.5亿年,对从最早的地质旋回开始到寒武纪起点这样一个长达34亿年、占地球历史八分之七的前寒武纪的研究已被人们放到了一个相当重要的地位。前寒武纪的研究,特别是前寒武纪地层学和古生物学的研究,关系到地球和地壳的形成与发展、大气圈和水圈的产生与变化、生命的起源和进化等等一系列带根本性的问题。  相似文献   

5.
全球范围内已确认的新生代陨击天文事件有8次,根据陨击直接证据或板块构造演化等推测的陨击事件至少还有3次,这些陨击天文事件都对应了新生代不同程度的气候变化。新生代全球气候变化的触发因素主要包括陨击天文事件、地球轨道参数变化、CO2浓度降低和全球碳循环变化、海洋及大气系统大量甲烷水合物释放、洋流变化及全球规模的构造运动(如构造隆升、超地幔柱、大规模火山活动)等,陨击天文事件是全球气候变化最主要的触发因素。  相似文献   

6.
23±0.3亿年(23.3~22.88亿年)时,地质环境(沉积圈、生物圈、水圈、大气圈)发生了由地外因素引起的灾变。灾变后,火山活动明显减弱,富氧大气圈形成,生物演化出现飞跃,气温骤降;进而引起一系列岩石、矿床、地球化学等方面的变化,并在全球范围有明显的一致性。所在,灾变是理想的地史分期界线,可作为太古宙—元古宙的分界。  相似文献   

7.
<正>地球上的生命起源于35亿年前,真核生物在20亿年前出现,多细胞生命在8~6亿年前出现,他们的出现均与地球表面的氧化作用有关。接下来5.4~5.2亿年前的"寒武纪生命大爆发"尽管在半个世纪前就被认为是氧含量的增加导致,但是在早寒武纪海洋的氧化还原条件,尤其是深海条件,仍处于争论。南京大学和苏黎世联邦理工学院最新研究发现"寒武纪生命大爆发"与全球海洋含氧底水的扩散保持一致。由于  相似文献   

8.
条带状铁建造(BIF)与地球大氧化事件   总被引:10,自引:0,他引:10       下载免费PDF全文
地球大氧化事件是指约24亿年前的地球大气圈中开始出现氧并连续增加。到20世纪末对地球大氧化事件的形成和演化模型可概括为两类:22亿年前为缺氧大气圈,22~19亿年大气圈中O_2明显增加,而后逐渐增加到现代大气圈O_2含量水平的C-W-K-H模型;大气圈中O_2含量自40亿年来近于常数,在现代大气圈O_2含量水平的50%范围内变化的D-K-O模型。21世纪开始实施了太古宙生物圈钻探计划(ABDP),在太古宙—元古宙页岩、条带状铁矿建造中微生物、S、C同位素分馏、稀土元素及过渡族金属Ni、Fe、Mo等含量变化等方面取得了许多新成果,建立了大气圈游离氧产生机理及含量变化的不同模型,将大气圈中氧的出现时间至少提前到25亿年前。中国前寒武纪条带状铁矿建造BIF广泛发育,特别是特有的稀土铁建造及其稀土地球化学初步研究成果表明,稀土元素的含量、轻重稀土的分异及变价元素Eu的相对富集与亏损,均显示明显的对时间的依赖。文中提出,应对其开展系统地质地球化学研究,可为大气圈、水圈的演化,特别是对研究中国铁矿的形成和分布规律研究提供重要参考资料。  相似文献   

9.
地壳上石撞击所引起陨的冲击变形是自然界一种快速变形现象,它具有许多与其它正常地质形变不尽相同的应变特征。笔者在收集国内外有关资料的基础上,对陨击成因的构造岩石类型及其划分,尤其是构造岩中的常见主要矿物的形变和相变特征进行了总结。它们可作为寻找古陨击坑、研究与陨击作用有关的成岩、成矿作用以及古深源地震方面的构造岩石学的标志。深入地研究地壳陨击构造岩的形变和相变,对于了解地球的发展演化有着重要的意义。  相似文献   

10.
史晓颖 《地球科学》1996,21(3):235-242
在地球过程中存在着35Ma的旋回周期,它不仅表现在全球性海平面变化,生物集群绝灭,构造运动幕,岩浆旋回以及古气候变化方面,而且也反映在古地磁倒转和陨击事件方面,反映了地球演化的自然阶段,重鄄质事件明显地集中于特定时期,形成自然临界,其可能主天体运行周期的控制,与太阳系穿越银道面有关。  相似文献   

11.
Kent Brooks 《Geology Today》2012,28(4):144-146
Throughout Earth history there have been many important milestones: e.g. the emergence of life, the rise of oxygen in the atmosphere, snowball Earth events. One of these major events was the emergence of multicellular life, which, as we are all told in Palaeontology lectures, took place in the Cambrian, when a sudden flowering of life forms emerged, including all of the major groups we have today: the ‘Cambrian explosion’. Two great questions emerge: what happened before this (a problem which worried Darwin as it seemed to threaten his thesis of steady evolution) and how, in detail did this ‘explosion’ take place?  相似文献   

12.
寒武纪生命扩张及澄江动物群的意义   总被引:1,自引:0,他引:1  
生命在地球上的出现及其演化有较长的历史。地球的物理、化学条件是早期生命出现的外因。早寒武世西南地区地质、气候及富含营养的浅海水域是澄江动物群在后生动物演化的关键时期出现的外因。“寒武纪生物的扩张”应有恰当的翻译,同时对现代生物学的“适应辐射”应有清楚的中文解释。从新近发现看,早、中寒武世的澄江动物群及布吉斯页岩动物群与埃迪卡拉动物群具有一些联系,埃迪卡拉动物群并没有在寒武纪时完全绝灭。  相似文献   

13.
舒德干  韩健 《地学前缘》2020,27(6):1-27
澄江动物群以富含多门类精美软躯体构造化石享誉学界,是寒武纪大爆发主幕的见证者;它亲眼目睹了地球动物树上几乎所有主要门类祖先的首次大聚会。对该动物群30多年的大规模调查研究大体上可以划分为3个阶段。始自1984年的第一个10年(1984—1994年),早期动物树上的基础动物亚界和原口动物亚界的大量门类被发现,然而对后口动物亚界全然无知。第二个10年研究(1995—2005年),基础动物亚界和原口动物亚界中的更多门类被发现;而最重要的进展,是西北大学团队主导的早期后口动物大发现使后口动物亚界的基本框架被构建,由此地球三分动物树首次成型。第三个10年及其以后时期(2005年之后),3个动物亚界中进一步添加了一些新的门类认知;综合20世纪40年代以来对埃迪卡拉生物群、寒武纪第一世和第二世的珍稀动物群研究成果,学界开始思考三分动物树分步成型与多幕式寒武纪大爆发事件的内在关联,提出了三幕式寒武纪大爆发新假说。澄江动物群研究具有多方面的科学价值,包括动物群结构研究,生态环境研究等,然其核心学术价值主要集中在如下两个方面:(1)作为寒武纪大爆发的主幕见证者,澄江动物群首次创建了地球上三分动物树的完整谱系框架。三幕式寒武纪大爆发假说揭示了地球上动物门类由低等到高等、分阶段爆发创造的本质内涵,即历时约0.4亿年的三幕式寒武纪大爆发与动物树阶段性快速成型的内在耦合性。第一幕发生于埃迪卡拉纪晚期,它诞生了众多基础动物亚界门类(包括大量绝灭门类),也可能出现了少量原口动物的先驱分子;第二幕发生于寒武纪的第一世,除了延续基础动物门类的繁盛外,更创生了原口动物亚界里的主要门类(包括蜕皮类和触手担轮类);第三幕发生于寒武纪第二世(以澄江动物群为代表),不仅延续了基础动物和原口动物门类的兴盛,更重要的是诞生了后口动物亚界里的所有门类。至此,整个三分动物树的框架成型,寒武纪大爆发创新事件宣告基本结束。文章还对几个重要动物类群的生物学属性进行了评述。第一鱼昆明鱼目是已知唯一的最古老脊椎动物,而云南虫、海口虫既不是脊椎动物(即高等脊索动物),也不属于低等脊索动物,而是一类特殊的低等后口动物;长江海鞘是可信的始祖尾索动物,它支持了经典的尾索动物起源假说;古虫动物门首创鳃裂构造,对后口动物亚界的起源探索提供了关键信息。(2)澄江动物群具有深刻的人文哲学意义,所发现的古虫动物门创造的“第一鳃裂”,昆明鱼目创造的“第一头脑”“第一脊椎”“第一心脏”,为达尔文在《人类的由来》中关于人类的主要基础器官起源悬案的破解提供了关键证据。澄江动物群承上启下,其各种形态解剖学信息对解读埃迪卡拉生物群以及寒武纪相关化石库中绝大多数生物类型都具有重要的参考价值。  相似文献   

14.
新元古代”雪球”假说与生命演化的环境   总被引:2,自引:0,他引:2  
新元古代末期,地球至少经历了两次全球性的冰川作用,研究者提出了“雪球”假说来解释新元古代时期一系列特殊的地质现象,该假说已成为研究新元古代全球冰川作用和其后生物大爆发事件的窗口。但一些学者并不赞成地球曾经是被冰雪完全覆盖的“雪球”,并分别提出了“半融雪球/无冰水体”和“薄冰”假说。尽管每一种假说都不能解释所有的地质、地球化学现象,但越来越越多的证据,特别是分子有机地球化学和古生物学的证据表明,“雪球”时期的海洋并没有完全被冰封盖,在赤道地区的冰盖可能很薄或存在无冰的水体。无冰水体的存在可以使一些光合生物继续生存和演化,这对其后的“寒武纪生物大爆发”事件和生命演化具有重要的意义。  相似文献   

15.
《Earth》2008,88(3-4):61-93
Sedimentological observations and palaeomagnetic data for Cryogenian glacial deposits present the climatic paradox of grounded glaciers and in situ cold climate near sea-level, glaciomarine deposition, and accompanying large (up to 40 °C) seasonal changes of temperature, all in low to near-equatorial (< 10°) palaeolatitudes (equated with geographic latitudes). Neither the “snowball Earth” nor the “slushball Earth” hypothesis can account for such strong seasonality near the palaeoequator, which together with findings from sedimentology, chemostratigraphy, biogeochemistry, micropalaeontology, geochronology and climate modelling argue against those scenarios. An alternative explanation of glaciation and strong seasonality in low palaeolatitudes is offered by a high (> 54°) obliquity of the ecliptic, which would render the equator cooler than the poles, on average, and amplify global seasonality. A high obliquity per se would not have been a primary trigger for glaciation, but would have strongly influenced the latitudinal distribution of glaciers. The principle of low-latitude glaciation on a terrestrial planet with high obliquity is validated by theoretical studies and observations of Mars. A high obliquity for the early Earth is a likely outcome of a single giant impact at 4.5 Ga, the widely favoured mechanism for lunar origin. This implies that a high obliquity could have prevailed during most of the Precambrian, controlling the low palaeolatitude of glaciations in the early and late Palaeoproterozoic and Cryogenian. It is postulated that the obliquity changed to < 54° between the termination of the last Cryogenian low-palaeolatitude glaciation at ≤ 635 Ma and the initiation of Late Ordovician–Early Silurian circum-polar glaciation at 445 Ma.The High Obliquity, Low-latitude Ice, STrong seasonality (HOLIST) hypothesis for pre-Ediacaran glaciation emerges favourably from numerous glacial and non-glacial tests. The hypothesis is in accord with such established or implied features of Cryogenian glaciogenic successions as extensive and long-lived open seas, an active hydrological cycle, aridity and palaeowesterly (reversed zonal) winds in low palaeolatitudes, and the apparent diachronism or non-correlation of some low-palaeolatitude glaciations. A pre-Ediacaran high obliquity also offers a viable solution of the faint young Sun paradox of a warm Archaean Earth. Furthermore, reduction of obliquity during the Ediacaran–early Palaeozoic would have yielded a more habitable globe with much reduced seasonal stresses and may have been an important factor influencing the unique evolutionary events of the Ediacaran and Cambrian. The palaeolatitudinal distribution of evaporites cannot discriminate unambiguously between high- and low-obliquity states for the pre-Ediacaran Earth. Intervals of true polar wander such as postulated by others for the Ediacaran and Early Cambrian imply major mass-redistributions within the Earth at those times, which may provide a potential mechanism for reducing the obliquity during the Ediacaran–early Palaeozoic.  相似文献   

16.
《Gondwana Research》2014,25(3):910-944
For life to have dramatically evolved and diversified during the so-called Cambrian explosion, there must have been significant changes in the environmental conditions of Earth. A rapid increase in atmospheric oxygen, which has been discussed as the key factor in the evolution of life, cannot by itself explain such an explosion, since life requires more than oxygen to flourish let alone survive. The supply of nutrients must have played a more critical role in the explosion, including an increase in phosphorus (P) and potassium (K) which are key elements for metabolisms to function. So, what happened at the onset of the Cambrian to bring about changes in environmental conditions and nutrient supply and ultimately evolution of life?An ultimate trigger for the Cambrian explosion is proposed here. The geotherm along subduction zones of a cooling Earth finally became cool enough around 600 Ma to allow slabs to be hydrated. The subduction of these hydrated slabs transferred voluminous water from the ocean to the mantle, resulting in a lowering of the sea level and an associated exceptional exposure of nutrient-enriched continental crust, along with an increase in atmospheric oxygen. This loss of water at the surface of the Earth and an associated increase in exposed landmass is referred to here as leaking Earth. Vast amounts of nutrients began to be carried through weathering, erosion, and transport of the landmass; rock fragments of the landmass would break down into ions during transport to the ocean through river, providing life forms (prokaryote) sufficient nutrients to live and evolve. Also, plume-driven dome-up beneath the continental crusts broadened the surface area providing a supply of nutrients an order magnitude greater than that produced through uplift of mountains by continental collision. Simultaneously, atmospheric oxygen began to increase rapidly due to the burial of dead organic matter by enhanced sedimentation from the emergence of a greater landmass, which ultimately inhibited oxidation of organic matter. Hence, oxygen began to accumulate in the atmosphere, which when coupled with a continuous supply of nutrients, resulted in an explosion of life, including an increase in the size. An enhanced oxygen supply in the atmosphere resulted in the formation of an ozone layer, providing life a shield from the UV radiation of the Sun; this enabled life to invade the land. In addition to a change in the supply of nutrients related to a leaking Earth, the evolution of life was accelerated through mass extinction events such as observed during Snowball Earth, possibly related to a starburst in our galaxy, as well as mutation in the genome due to radiogenic elements sourced from carbonatite magma (atomic bomb magma) in rift valley. There are two requirements to find a habitable planet: (1) the initial mass of an ocean and (2) the size of a planet. These two conditions determine the history of a planet, including planetary tectonics and the birth of life. This newfound perspective, which includes the importance of a leaking planet, provides a dawn of new planetary science and astrobiology.  相似文献   

17.
冰雪地球的研究进展综述   总被引:3,自引:0,他引:3  
胡永云  闻新宇 《地球科学进展》2005,20(11):1226-1233
在大约6~7亿年前的新元古代时期,地球是否曾经被冰雪完全覆盖而成为了一个“冰雪地球”?如果是,什么诱发了这种全球性的冰川期?又是什么导致了它的融化?新元古代时期的极端气候变化对其后的寒武纪生命大爆发有何影响?围绕这些问题,古地质、古生物和古气候学界在最近几年展开了广泛的研究和激烈争论。根据现有的研究结果,地球在新元古代时期确实经历了数次地球历史上最为严重的全球性冰川期,但地球是否被完全冰封还需要更充分的古地质和古生物方面的证据来证明;利用气候模式对各种可能的外部强迫的模拟试验表明“冰雪地球”是很难形成的,并且,如果地球进入完全被冰封的状态,它将是难以被融化的;关于新元古代时期剧烈的气候变化对寒武纪生命大爆发所起的作用存在2种观点,一种认为气候变化导致了原始生命的基因突变并诱发了寒武纪生命爆发,另一种认为这种影响主要是生态方面的。  相似文献   

18.
《Gondwana Research》2014,25(3):945-965
The birth of modern life on Earth can be linked to the adequate supply of nutrients into the oceans. In this paper, we evaluate the relative supply of nutrients into the ocean. These nutrients entered the ocean through myriad passageways, but primarily through accelerated erosion due to uplift. In the ‘second ecosystem’, uplift is associated with plume-generation during the breakup of the Rodinia supercontinent. Although the evidence is somewhat cryptic, it appears that the second ecosystem included the demospongia back into the Cryogenian (~ 750 Ma). During the Ediacaran–Cambrian interval, convergent margin magmatism, arc volcanism and the closure of ocean basins provided a second pulse of nutrient delivery into the marine environment. A major radiation of life forms begins around 580 Ma and is represented by the diverse and somewhat enigmatic Ediacaran fauna followed by the Cambrian Explosion of modern phyla during the 540–520 Ma interval. Tectonically, the Ediacaran–Cambrian time interval is dominated by the formation of ultra-high pressure (UHP), high pressure (HP) and ultra-high temperature (UHT) orogenic belts during Gondwana orogenesis. Erosion of this extensive mountainous region delivered vast nutrients into the ocean and enhanced the explosiveness of the Cambrian radiation. The timing of final collisional orogeny and construction of the mountain belts in many of the Gondwana-forming orogens, particularly some of those in the central and eastern belts, post-date the first appearance of modern life forms. We therefore postulate that a more effective nutrient supply for the Cambrian radiation was facilitated by plume-driven uplift of TTG crust, subsequent rifting, and subduction-related nutrient systems prior to the assembly of Gondwana. In the outlined scenario, we propose that the birth of the ‘second ecosystem’ on our planet is plume-driven.  相似文献   

19.
Life was limited for most of Earth's history, remaining at a primitive stage and mostly marine until about 0.55 Ga. In the Paleozoic, life eventually exploded and colonized the continental realm. Why had there been such a long period of delayed evolution of life? Early life was dominated by Archaea and Bacteria,which can survive ionizing radiation better than other organisms. The magnetic field preserves the atmosphere, which is the main shield of UV radiation. We explore the hypothesis that the Cambrian explosion of life could have been enabled by the increase of the magnetic field dipole intensity due to the solidification of the inner core, caused by the cooling of the Earth, and the concomitant decrease with time of the high-energy solar flux since the birth of the solar system. Therefore, the two phenomena could be responsible for the growth and thickening of the atmosphere and the development of land surface life.  相似文献   

20.
The radiation of macroscopic animals in the Early Cambrian, commonly be called as ‘Cambrian explosion’, had a close relationship with Earth oxygenation. These macrofossils are widely preserved within the Early Cambrian in the northern and western Yangtze Craton. In order to show the casual relationship between animal evolution and Earth redox environment, Mo content and isotopic composition analyses have been conducted on dolomites of the Tianzhushan Formation and the black shales of the Shuijingtuo Formation from the lowermost Cambrian profile in the eastern Huangling dome, northern Yangtze Craton. The calcitic dolostones from the Tianzhushan Formation display lower concentrations of Mo contents (0.055–0.666 ppm) than that of the black silty shales from the Shuijingtuo Formation (6.0–172 ppm). This magnitude difference is most likely related to the different lithologies due to Mo enrichment in shales. The Mo isotope values (δ98/95Mo) of the calcitic dolostones for the Tianzhushan Formation vary from −0.73‰ to 0.41‰. In comparison, the black sandy shales from the Shuijingtuo Formation exhibit δ98/95Mo of −1.04–1.84‰, including 5 samples from the earliest Shuijingtuo Formation displaying systematically higher δ98/95Mo values (0.09–1.84‰) than those of the other 5 samples from upper layers (δ98/95Mo = −1.04 to −0.19‰). These geochemical data suggest that the redox environment of the early Cambrian is fluctuating, and the peak oxygenation of the ocean had already reached a level similar to modern environments. According to the Mo concentrations and δ98/95Mo data, the sedimentary succession can be divided into five intervals, which are closely correlated to the episodic evolution of early life in the Cambrian. Together with the available published data from other profiles in the Yangtze Craton, our new data reveal that the higher oxidation environment had a positive effect on the evolution of early life.  相似文献   

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