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1.
澳大利亚西北陆架贫油富气,在近年的勘探开发中显示出广阔的前景.通过对澳大利亚西北陆架大量相关文献的分析总结,区域上包括4个盆地和1个造山带:北卡那封盆地、柔布克盆地、布劳斯盆地、渡拿巴盆地和帝汶-班达褶皱带.西北陆架属边缘海型被动大陆边缘,构造演化经历了前裂谷期、裂谷期和被动大陆边缘期三大阶段,对应发育有三大沉积建造层... 相似文献
2.
《海洋地质与第四纪地质》2015,(1)
澳大利亚西北陆架盆地是一个长期继承性发育的叠合盆地,三叠纪时期处于稳定克拉通大陆边缘拗陷阶段,沉积区基底构造稳定,坡度平缓,发育大型的浅水三角洲。利用钻井、地震以及古生物资料,明确了当时的古地理、古气候与沉积特征:平面上具有三角洲平原分布广、三角洲前缘欠发育、无前积现象等特征;纵向上具有相漂移、地层厚度大、三角洲平原薄煤层普遍发育等特点;沉积作用以单向水流作用为主,正旋回的分支流水道砂体广泛发育;三角洲砂岩分布广,成分成熟较高,但分选磨圆差—中等,互层泥岩中陆源碎屑有机组分丰富,体现了浅水、快速堆积、远距离搬运的特点。平面上西北陆架North Carnarvon以及Browse主力三角洲砂体位于中晚三叠世卡尼期—诺瑞期;而Bonaparte盆地主力砂体位于中三叠世拉丁期—卡尼期。晚三叠世澳大利亚西北陆架北部普遍发生抬升,导致Browse盆地与Bonaparte盆地三叠系发育不全,三角洲规模较小;而西北陆架西南部North Carnarvon盆地地层发育齐全,厚度大,且发育大型三角洲。Pilbara地块、Yilgarn地块以及Kimberley地块为源区三大古陆,其中Pilbara地块与Yilgarn地块大多出露太古代花岗岩类,Kimberley地块以元古代变质结晶岩和沉积岩为主,为盆地提供了充足的碎屑沉积物。利用岩矿资料、磷灰石裂变径迹等资料探讨了大型三角洲的碎屑物来源:North Carnarvon盆地物源主要来自于Pilbara以及Yilgarn地块,Browse以及Bonaparte盆地物源主要来自于Kimberley地块。研究成果表明,在三叠纪全球温室气候背景条件下,特提斯南缘具有发育大型三角洲的特殊古地理背景;大型三角洲发育的地质条件除充足的降雨与丰富的物源供给外,还必须具有稳定持续沉降的构造背景。 相似文献
3.
澳大利亚西北陆架中生界生储盖组合特征 总被引：6，自引：0，他引：6
澳大利亚西北陆架是一个贫油富气的地区,在近年的勘探开发中显示出广阔的前景。区域上包含4个盆地和1个造山带:北卡那封盆地、柔布克盆地、布劳斯盆地、波拿巴盆地和帝汶—班达褶皱带。西北陆架油气绝大多数集中在中生界。中生界发育4套主要烃源岩:三叠系湖相泥页岩、下—中侏罗统海相和海陆交互相碳质泥岩和煤系、上侏罗统海相页岩及下白垩统海相泥页岩;主要储集岩为中—上三叠统三角洲—边缘海相砂岩、下—中侏罗统砂岩、上侏罗统砂岩和白垩系砂岩;主要区域性盖层是下白垩统海相泥页岩。根据生储盖组合的沉积环境,主要发育海生海储海盖型和陆生陆储陆盖型两大生储盖组合类型。海生海储海盖型生储盖组合广泛分布于西北大陆架,是区域最重要的成藏组合。 相似文献
4.
《海洋地质与第四纪地质》2010,(4)
南海北部陆坡区的台西南盆地是天然气水合物潜在分布区之一,水合物稳定带的研究对天然气水合物成矿与分布规律以及资源评价都具有重要意义,根据SO-177中德合作航次南海北部陆坡天然气水合物地质的调查资料,结合天然气水合物的相平衡条件和相应的压力-温度方程,计算了台西南盆地A区和B区的水合物稳定带厚度,并讨论了水合物稳定带厚度的分布特征。另外,对A区和B区天然气水合物中甲烷资源量进行了初步估算,估算结果为:A区甲烷资源含量为8.5739×1011～5.1443×1012m3,B区甲烷资源含量为1.4518×1012～8.7111×1012m3,A区和B区甲烷资源总量约2.3029×1012～13.8544×1012m3。初步估算结果显示,台西南盆地天然气水合物甲烷资源量潜力巨大。 相似文献
5.
世界主要深水含油气盆地储层特征 总被引：3，自引：0，他引：3
世界深水盆地油气资源丰富,良好的储层是形成较大油气藏的必要条件.以大量调研资料为基础,对大西洋区域的墨西哥湾、巴西东部边缘、非洲西海岸、挪威中部陆架及新特提斯区域的澳大利亚西北陆架、中国南海、孟加拉湾、地中海(尼罗河三角洲)8个地区的24个深水含油气盆地储层特征进行了综合分析,归纳总结了这些深水含油气盆地中主力储层的形... 相似文献
6.
7.
珠江口和琼东南盆地天然气水合物形成和稳定分布的地球化学边界条件及其分布区 总被引：22，自引：0，他引：22
通过对南海北部陆缘珠江口和琼东南盆地气田的天然气形成水合物的地球化学计算模拟及地质地球化学条件分析，对珠江口和琼东南盆地天然气形成水合物的地球化学边界条件及分布区进行了研究。认识到南海北部陆缘琼东南和珠江口盆地内的断裂构造是天然气向海底渗漏的通道，为天然气水合物在海底的形成提供了物源；盆地内巨厚的第四纪富有机质沉积也为天然气水合物形成提供了充足的细菌成因生物气源。在海底温度2－16℃范围内，琼东南盆地气田10种天然气和珠江口盆地气田18种天然气形成水合物的压力有比较大的范围，随温度增高，天然气水合物形成的压力增高；盆地间和各天然气样品之间形成水合物的压力均是不一致的。在南海海水平均盐度3．4％条件下，结合海底温度与水深变化资料，珠江口和琼东南盆地天然气水合物形成和稳定分布的海区是不同的，珠江口盆地小于230m水深的海区没有天然气水合物的形成，在230－760m水深的海区可能有天然气水合物的存在，天然气水合物的稳定分布区应该在大于860m水深的深水区；在琼东南盆地水深小于320m的海区不可能有天然气水合物的形成，在320－650m水深的海区可能有天然气水合物的存在，大于650m水深的海区是天然气水合物的稳定分布区。 相似文献
8.
南设得兰陆缘属于典型的活动型大陆边缘,沟-增生楔-弧前盆地序列发育,具备天然气水合物发育的有利地质构造背景。该区已有的调查资料显示出天然气水合物存在的显著标志——BSR和极性反转特征(或者称为基底反射波,BGR)。研究结果表明,南设得兰陆缘具备形成水合物的充足的气源、适宜的稳定域条件、有利于天然气水合物形成与聚集的沉积体系和特殊地质构造环境,推断南设得兰陆缘以构造型水合物成矿地质模式为主,并以增生楔内甲烷随流体向上迁移形成水合物的模式最为重要。 相似文献
9.
位于南极半岛西侧的别林斯高晋海是南极附近海域天然气水合物成矿的远景区域。利用现有钻孔岩心样品、地震剖面、声波等资料,从气源、稳定域、构造输导及沉积储集等方面,分析了别林斯高晋海天然气水合物的形成条件,预测了天然气水合物成矿远景区,初步探讨了其形成机理,以期能为今后南极半岛区域的天然气水合物资源调查研究提供一定的科学参考依据。 相似文献
10.
针对天然气水合物沉积成矿因素不明确等问题,通过利用南海北部神狐海域的高分辨率三维地震、测井和岩心等资料,对晚中新世以来的地层进行了高分辨率层序划分和精细的沉积解释。从温压、沉积、构造等方面探讨了神狐海域天然气水合物分布的主控因素,认为：BSR上部附近处于水合物稳定温压范围内;粗粒沉积物有利于天然气水合物的富集;在含水合物层段内,孔隙度与天然气水合物饱合度成正比关系;滑塌体是天然气水合物赋存的有利相带;气烟囱形成过程中产生的断裂系统可为富含甲烷流体向上运移提供通道,并在其上部滑塌体富集成矿。因此,神狐海域具备天然气水合物成藏的优越条件,是天然气水合物勘探开发的有利区块。 相似文献
11.
On the southwestern Barents Sea shelf, sediments containing gas hydrates that overlie free gas have been inferred from multichannel
seismic data. The volume of suspected gas hydrate is tentatively estimated to about 1.9×108 m3. The gas hydrate zone probably formed from thermogenic gas leaking from a deeper source. The hydrate zone may have thickened
during the Neogene by including gas originally trapped as free gas below the hydrate following a significant downward migration
of the isotherms caused by erosion and/or subsidence. Within the present oceanographic conditions, gas hydrate is suspected
to be stable or slowly decomposing.
Received: 20 December 1996 / Revision received: 20 August 1997 相似文献
12.
The South China Sea (SCS) shows favorable conditions for gas hydrate accumulation and exploration prospects. Bottom simulating reflectors (BSRs) are widely distributed in the SCS. Using seismic and sequence stratigraphy, the spatial distribution of BSRs has been determined in three sequences deposited since the Late Miocene. The features of gas hydrate accumulations in northern SCS were systematically analyzed by an integrated analysis of gas source conditions, migration pathways, heat flow values, occurrence characteristics, and depositional conditions (including depositional facies, rates of deposition, sand content, and lithological features) as well as some depositional bodies (structural slopes, slump blocks, and sediment waves). This research shows that particular geological controls are important for the presence of BSRs in the SCS, not so much the basic thermodynamic controls such as temperature, pressure and a gas source. Based on this, a typical depositional accumulation model has been established. This model summarizes the distribution of each depositional system in the continental shelf, continental slope, and continental rise, and also shows the typical elements of gas hydrate accumulations. BSRs appear to commonly occur more in slope-break zones, deep-water gravity flows, and contourites. The gas hydrate-bearing sediments in the Shenhu drilling area mostly contain silt or clay, with a silt content of about 70%. In the continental shelf, BSRs are laterally continuous, and the key to gas hydrate formation and accumulation lies in gas transportation and migration conditions. In the continental slope, a majority of the BSRs are associated with zones of steep and rough relief with long-term alternation of uplift and subsidence. Rapid sediment unloading can provide a favorable sedimentary reservoir for gas hydrates. In the continental rise, BSRs occur in the sediments of submarine fans, turbidity currents. 相似文献
13.
P. Dewangan T. RamprasadM.V. Ramana A. MazumdarM. Desa F.K. Badesab 《Marine and Petroleum Geology》2010
Increased oil and gas exploration activity has led to a detailed investigation of the continental shelf and adjacent slope regions of Mahanadi, Krishna–Godavari (KG) and Cauvery basins, which are promising petroliferous basins along the eastern continental margin of India. In this paper, we analyze the high resolution sparker, subbottom profiler and multibeam data in KG offshore basin to understand the shallow structures and shallow deposits for gas hydrate exploration. We identified and mapped prominent positive topographic features in the bathymetry data. These mounds show fluid/gas migration features such as acoustic voids, acoustic chimneys, and acoustic turbid layers. It is interesting to note that drilling/coring onboard JOIDES in the vicinity of the mounds show the presence of thick accumulation of subsurface gas hydrate. Further, geological and geochemical study of long sediment cores collected onboard Marion Dufresne in the vicinity of the mounds and sedimentary ridges shows the imprints of paleo-expulsion of methane and sulfidic fluid from the seafloor. 相似文献
14.
南海天然气水合物的形成和分布 总被引：17，自引：0，他引：17
姚伯初 《海洋地质与第四纪地质》2005,25(2):81-90
从物理海洋、古气候、沉积环境和构造环境分析入手，研究了南海天然气水合物的形成条件。研究结果表明，在整个南海海域，天然气水合物生成的条件是存在差别的。南海，东北部，在氧同位素2、4、6期，由于菲律宾海的高盐度海水的注入，使这里的生物生产率特别高，陆坡上沉积了丰富的有机物质，加上此期间该处的沉积速率高，为天然气水合物的生成提供了物质条件；另外，自中新世末以来，由于菲律宾海板块与欧亚板块在台湾地区发生碰撞，对南海北部产生北西向挤压，加快了流体在沉积物中的活动，为天然气水合物的生成提供了良好的构造环境。因此认为南海东北部陆坡应是南海天然气水合物最丰富的地区。 相似文献
15.
沉积盆地内能够形成天然气水合物的先决条件包括：富含分散有机质的沉积物中充有地下水、深水区的水动力处于滞流状态、存在生物成因的气体、压力与温度具有特定的相关关系等。许多科学家提出天然气水合物主要有两种成因机制：（1）先存天然气田因温度或孔隙压力的有利变化而转变为天然气水合物；（2）微生物成因气或热成因气从下部运移至天然气水合物稳定带。 相似文献
16.
S. Chand L. RiseJ. Knies H. HaflidasonB.O. Hjelstuen R. Bøe 《Marine and Petroleum Geology》2011,28(7):1350-1363
The Cenozoic seismic stratigraphy and geological development of the south Vøring margin are analyzed to understand their relation to fluid flow and margin stability. The regional stratigraphy and palaeomorphology of the Møre and Vøring basins indicate gradual changes in depositional environment and tectonic compression between 55 Ma to 2.8 Ma during Brygge and Kai periods, and abrupt changes associated with glacial/interglacial cycles from last 2.8 Ma during Naust period. These changes resulted in deposition of various types of sediments and led to processes such as polygonal faulting and dewatering, inter-fingering of contouritic, stratified and glacigenic sediments, and margin progradation.A gas hydrate related bottom simulating reflector (BSR) occurs at Nyegga and within the central Vøring Basin while pockmarks are observed at Nyegga only. Diagentic reflectors due to Opal A - Opal CT conversion (DBSRs) occur along a wider area beyond the shelf edge. The DBSRs are located in oozes within the Kai and late Brygge Formations. The gas hydrate BSR occurrence is concentrated above Eocene depocenters in hemipelagic and contouritic sediments deposited during Late Plio-Pleistocene. The BSR overlies polygonal faults and DBSRs but are confined to the slope of anticlines indicating its formation being related to fluid pathways from methanogenic rocks through focused fluid flow. Microbial gas production in Kai, Brygge and deeper formations may have supplied the gas for gas hydrate formation. Fluid expulsion due to DBSR formation and polygonal faulting in oozes may have created overpressure development in permeable layers belonging to the overlying Naust Formation. Slide headwalls are also located close to the anticlines in the study area, implying that over pressured oozes and focussed fluid flow may have been important in creating weak surfaces in the overlying Naust sediments, promoting conditions for failures to occur. 相似文献
17.
Catherine Pierre Marie-Madeleine Blanc-Valleron Jér?me Demange Omar Boudouma Jean-Paul Foucher Thomas Pape Tobias Himmler Noemi Fekete Volkhard Spiess 《Geo-Marine Letters》2012,32(5-6):501-513
The southwest African continental margin is well known for occurrences of active methane-rich fluid seeps associated with seafloor pockmarks at water depths ranging broadly from the shelf to the deep basins, as well as with high gas flares in the water column, gas hydrate accumulations, diagenetic carbonate crusts and highly diverse benthic faunal communities. During the M76/3a expedition of R/V METEOR in 2008, gravity cores recovered abundant authigenic carbonate concretions from three known pockmark sites—Hydrate Hole, Worm Hole, the Regab pockmark—and two sites newly discovered during that cruise, the so-called Deep Hole and Baboon Cluster. The carbonate concretions were commonly associated with seep-benthic macrofauna and occurred within sediments bearing shallow gas hydrates. This study presents selected results from a comprehensive analysis of the mineralogy and isotope geochemistry of diagenetic carbonates sampled at these five pockmark sites. The oxygen isotope stratigraphy obtained from three cores of 2–5?m length indicates a maximum age of about 60,000–80,000?years for these sediments. The authigenic carbonates comprise mostly magnesian calcite and aragonite, associated occasionally with dolomite. Their very low carbon isotopic compositions (–61.0?<?δ13C ‰ V-PDB?<?–40.1) suggest anaerobic oxidation of methane (AOM) as the main process controlling carbonate precipitation. The oxygen isotopic signatures (+2.4?<?δ18O ‰ V-PDB?<?+6.2) lie within the range in equilibrium under present-day/interglacial to glacial conditions of bottom seawater; alternatively, the most positive δ18O values might reflect the contribution of 18O-rich water from gas hydrate decomposition. The frequent occurrence of diagenetic gypsum crystals suggests that reduced sulphur (hydrogen sulphide, pyrite) from sub-seafloor sediments has been oxidized by oxygenated bottom water. The acidity released during this process can potentially induce the dissolution of carbonate, thereby providing enough Ca2+ ions for pore solutions to reach gypsum saturation; this is thought to be promoted by the bio-irrigation and burrowing activity of benthic fauna. The δ18O–δ13C patterns identified in the authigenic carbonates are interpreted to reflect variations in the rate of AOM during the last glacial–interglacial cycle, in turn controlled by variably strong methane fluxes through the pockmarks. These results complement the conclusions of Kasten et al. in this special issue, based on authigenic barite trends at the Hydrate Hole and Worm Hole pockmarks which were interpreted to reflect spatiotemporal variations in AOM related to subsurface gas hydrate formation–decomposition. 相似文献
18.
A. Zabanbark 《Oceanology》2010,50(2):268-280
The oil and gas basins of Australia are confined to its western and northwestern margins. They are typical pericontinental
depressions in the continent-ocean transition zone with a passive tectonic regime. The following oil and gas basins are definable
from the south to northward: the Perth, Carnarvon, Canning, Browse, and Bonaparte. All these basins are well studied. Among
them, the Carnarvon basin is the most productive. Despite the discovery of approximately a hundred oil and gas fields in this
basin, its continental slopes are still insufficiently known. In this connection, the morphostructural features of the productive
areas were analyzed using a specialized GIS technique. The performed analysis of the Carnarvon hydrocarbon-bearing basin demonstrated
the efficiency of this technique and allowed several promising zones located west, north, and south of the discovered oil
and gas fields and forming a single trend with them to be outlined. The total reserves of the country are as high as 2.1 ×
109 t of oil and 840 × 109 m3 of gas. The annual oil production in Australia by January 1, 2008 was 22.25 × 106 t of oil and 14 × 109 m3 of gas. Approximately 95% of the oil and 80% of the gas produced in Australia by the beginning of 2008 were obtained from
offshore parts of its basins. 相似文献
19.
In this study we provide evidence for methane hydrates in the Taranaki Basin, occurring a considerable distance from New Zealand's convergent margins, where they are well documented. We describe and reconstruct a unique example of gas migration and leakage at the edge of the continental shelf, linking shallow gas hydrate occurrence to a deeper petroleum system. The Taranaki Basin is a well investigated petroleum province with numerous fields producing oil and gas. Industry standard seismic reflection data show amplitude anomalies that are here interpreted as discontinuous BSRs, locally mimicking the channelized sea-floor and pinching out up-slope. Strong reverse polarity anomalies indicate the presence of gas pockets and gas-charged sediments. PetroMod™ petroleum systems modelling predicts that the gas is sourced from elevated microbial gas generation in the thick slope sediment succession with additional migration of thermogenic gas from buried Cretaceous petroleum source rocks. Cretaceous–Paleogene extensional faults underneath the present-day slope are interpreted to provide pathways for focussed gas migration and leakage, which may explain two dry petroleum wells drilled at the Taranaki shelf margin. PetroMod™ modelling predicts concentrated gas hydrate formation on the Taranaki continental slope consistent with the anomalies observed in the seismic data. We propose that a semi-continuous hydrate layer is present in the down-dip wall of incised canyons. Canyon incision is interpreted to cause the base of gas hydrate stability to bulge downward and thereby trap gas migrating up-slope in permeable beds due to the permeability decrease caused by hydrate formation in the pore space. Elsewhere, hydrate occurrence is likely patchy and may be controlled by focussed leakage of thermogenic gas. The proposed presence of hydrates in slope sediments in Taranaki Basin likely affects the stability of the Taranaki shelf margin. While hydrate presence can be a drilling hazard for oil and gas exploration, the proposed presence of gas hydrates opens up a new frontier for exploration of hydrates as an energy source. 相似文献
20.
2D and 3D seismic reflection and well log data from Andaman deep water basin are analyzed to investigate geophysical evidence related to gas hydrate accumulation and saturation. Analysis of seismic data reveals the presence of a bottom simulating reflector (BSR) in the area showing all the characteristics of a classical BSR associated with gas hydrate accumulation. Double BSRs are also observed on some seismic sections of area (Area B) that suggest substantial changes in pressure–temperature (P–T) conditions in the past. The manifestation of changes in P–T conditions can also be marked by the varying gas hydrate stability zone thickness (200–650 m) in the area. The 3D seismic data of Area B located in the ponded fill, west of Alcock Rise has been pre-stack depth migrated. A significant velocity inversion across the BSR (1,950–1,650 m/s) has been observed on the velocity model obtained from pre-stack depth migration. The areas with low velocity of the order of 1,450 m/s below the BSR and high amplitudes indicate presence of dissociated or free gas beneath the hydrate layer. The amplitude variation with offset analysis of BSR depicts increase in amplitude with offset, a similar trend as observed for the BSR associated with the gas hydrate accumulations. The presence of gas hydrate shown by logging results from a drilled well for hydrocarbon exploration in Area B, where gas hydrate deposit was predicted from seismic evidence, validate our findings. The base of the hydrate layer derived from the resistivity and acoustic transit-time logs is in agreement with the depth of hydrate layer interpreted from the pre-stack depth migrated seismic section. The resistivity and acoustic transit-time logs indicate 30-m-thick hydrate layer at the depth interval of 1,865–1,895 m with 30 % hydrate saturation. The total hydrate bound gas in Area B is estimated to be 1.8 × 1010 m3, which is comparable (by volume) to the reserves in major conventional gas fields. 相似文献