Hydrocarbons generation potential of the Jurassic–Lower Cretaceous Formation, Ajeel field, Iraq

Organic geochemical analysis and palynological studies of the organic matters of subsurface Jurassic and Lower Cretaceous Formations for two wells in Ajeel oil field, north Iraq showed evidences for hydrocarbon generation potential especially for the most prolific source rocks Chia Gara and Sargelu Formations. These analyses include age assessment of Upper Jurassic (Tithonian) to Lower Cretaceous (Berriasian) age and Middle Jurassic (Bathonian–Tithonian) age for Chia Gara and Sargelu Formations, respectively, based on assemblages of mainly dinoflagellate cyst constituents. Rock-Eval pyrolysis have indicated high total organic carbon (TOC) content of up to 18.5 wt%, kerogen type II with hydrogen index of up to 415 mg HC/g TOC, petroleum potential of 0.70–55.56 kg hydrocarbon from each ton of rocks and mature organic matter of maximum temperature reached (T_max) range between 430 and 440 °C for Chia Gara Formation, while Sargelu Formation are of TOC up to 16 wt% TOC, Kerogen type II with hydrogen index of 386 mg HC/g TOC, petroleum potential of 1.0–50.90 kg hydrocarbon from each ton of rocks, and mature organic matter of T_max range between 430 and 450 °C. Qualitative studies are done in this study by textural microscopy used in assessing amorphous organic matter for palynofacies type belonging to kerogen type A which contain brazinophyte algae, Tasmanites, and foraminifera test linings, as well as the dinoflagellate cysts and spores, deposited in dysoxic–anoxic environment for Chia Gara Formation and similar organic constituents deposited in distal suboxic–anoxic environment for Sargelu Formation. The palynomorphs are of dark orange and light brown, on the spore species Cyathidites australis, that indicate mature organic matters with thermal alteration index of 2.7–3.0 for the Chia Gara Formation and 2.9–3.1 for the Sargelu Formation by Staplin's scale. These characters have rated the succession as a source rock for very high efficiency for generation and expulsion of oil with ordinate gas that charged mainly oil fields of Baghdad, Dyala (B?aquba), and Salahuddin (Tikrit) Governorates. Oil charge the Cretaceous-Tertiary total petroleum system (TPS) are mainly from Chia Gara Formation, because most oil from Sargelu Formation was prevented passing to this TPS by the regional seal Gotnia Formation. This case study of mainly Chia Gara oil source is confirmed by gas chromatography–mass spectrometry analysis for oil from reservoirs lying stratigraphically above the Chia Gara Formation in Ajeel and Hamrine oil fields, while oil toward the north with no Gotnia seal could be of mainly Sargelu Formation source.     

Applications of computer modeling to the study of the genesis of stratiform sulfide deposits

Stratiform sulfide deposits are considered to have formed at or near the discharge vents of submarine hydrothermal systems. Such deposits constitute an important source of zinc, lead, copper, silver, and gold. They are often divided on the basis of the dominant host-rock lithology into volcanogenic and sediment-hosted types. In terms of their economic base metal contents, volcanogenic deposits contain either Cu and Zn or Zn, Pb, and Cu, whereas sediment-hosted deposits usually contain predominantly Zn and Pb. Mathematical models of the chemical characteristics of stratiform sulfide deposits are based on a program (B)which allows the calculation of the equilibrium distribution of aqueous species in a hydrothermal solution. Program B is front-ended by Program A, which defines the components of the chemical system, and back-ended by Program C, which controls the mode of output of the calculated results. Programs A and C are tailored to the specific problem under investigation. Results of chemical modeling of the two chemically active zones of the hydrothermal system (1. the hydrothermal reservoir in which the ore-forming solutions are generated and, 2. the site of ore deposition)suggest explanations of various characteristics of stratiform sulfide deposits, and include

1. The consistency of the metal associations and metal ratios suggest that ore-forming hydrothermal solutions are saturated with respect to the major metals in the reservoir zone. The chemistry of the solutions is determined mainly by temperature and chemical equilibrium between the hydrothermal solution and the rock-forming minerals of the reservoir.
2. Metal associations and metal ratios corroborate isotopic and other evidence that volcanogenic deposits were formed from hotter hydrothermal systems (> 200°Capprox.)than sediment-hosted (< 200°Capprox.)Metal ratios suggest that the hydrothermal reservoirs were contained in mafic rocks (ferromagnesian-feldspar mineral assemblages)for the Cu-Zn association; in felsic rocks and/or sediments (feldspar-mica; clay mineral assemblages)for the Zn-Pb-Cu association: and in sediments (dominated by clay mineral assemblages)for the Zn-Pb association.
3. Chemical zonation patterns and ore textures characteristics of volcanogenic deposits are explained by rapid cooling of the hydrothermal solution immediately above its discharge vent.
4. Chemical zonation patterns and the fine laminations of sediment-hosted deposits are explained by the comparatively slow degeneration of hydrothermal solutions that have collected as a brine pool on the ocean floor.

     

Chain of galaxies in centaurus

Further photometric and spectroscopic observations of a chain of galaxies in Centaurus are presented and discussed.     

Using tornado climatology to help plan a Doppler radar network

Using the tornado climatology and population statistics for Canada, a method of ranking population centres is proposed. Using as a basis a list of cities and census divisions ranked by population-weighted tornado incidence (a measure of risk), a first estimate is made of where to site 22 Doppler radars. It is estimated that this network will provide protection to about 82% of Canada's population.     

Seed biology of Australian arid zone species: Germination of 18 species used for rehabilitation

Revegetation of disturbed land, particularly in arid environments, is often hindered by low seedling establishment. Information on seed biology and germination cues of keystone species is lacking, particularly in arid Australia; a major zone for mining developments. This study investigated seed characteristics and germination of 18 common species required for rehabilitation of disturbed areas at Shark Bay Salt in the Shark Bay World Heritage Area, Western Australia. Untreated seeds of seven species (Aphanopetalum clematideum, Atriplex bunburyana, Austrostipa elegantissima, Melaleuca cardiophylla, Pembertonia latisquamea, Rhagodia baccata, Salsola tragus) exhibited high germination percentages. Seeds of two species (Acacia tetragonophylla, Stylobasium spathulatum) had low imbibition, which increased with hot-water treatment, hence require scarification for germination. Gibberellic acid, smoke water and karrikinolide (a butenolide isolated from smoke) substantially increased germination percentages of three species (Anthocercis littorea, Diplolaena grandiflora, Solanum orbiculatum). Seeds of the remaining six species (Dioscorea hastifolia, Eremophila oldfieldii, Nitraria billardierei, Ptilotus exaltatus, Thryptomene baeckeacea, Zygophyllum fruticulosum) had low germination percentages regardless of treatment. Most species germinated equally well at 26/13 °C and 33/18 °C, however seven species had improved performance at 26/13 °C. This study is significant to land managers and conservation agencies with an interest in optimising germination of arid zone seeds for restoration.     

A detailed structural analysis of the Deslandres area of the Moon

The components of the Lunar grid of the Deslandres area of the Moon are described and their azimuths plotted. The grid is shown to be the product of endogenic processes which may also have been important in the early geological evolution of the Earth.     

Tensions in managing the suburbs: conservation versus change

Summary This paper rewiews the increasing trend for conservation in suburban areas. Focusing mainly on English suburban conservation areas, it explores the background to the movement, the views of residents and the range of town-planning systems used in such attempts to retain the 'character and appearance' of these areas. Concepts of, and approaches to, urban landscapes that might be familiar to urban geographers are conspicuous by their absence. A range of tensions are explored, including those generated between residents and professionals, the values and attitudes of the professionals and the likely future conflict over values and attitudes in conservation versus change: the application of concepts of sustainability, including 'densification' and the compact city.     

An unexploited population of oysters,Ostrea lutaria Hutton,from foveaux strait

Settlement of Ostrea lutaria on sand‐cement‐plastered asbestos plates held in steel frames on the bottom of Foveaux Strait was studied from March 1965 to April 1967. Spat mortality over the period of plate exposure (about one month) was very low (maximum of 3 percent) and was greatest shortly after settlement. There was no evidence that mortality was due to predation. Essentially the same seasonal pattern of settlement was observed each year. Eighty to 90 percent of spat settled between mid December and mid February in both summers; settlement occurred as early as October; some was observed as late as July.

Results of field experiments suggest some very tentative conclusions on the settlement behaviour of O. lutaria: (1) The larvae are benthopelagic and remain on the bottom in strong current conditions. (2) Light stimulates swimming of larvae in still water. (3) In still water and low light intensities of the area larvae tend to swim upward toward the light. (4) In still water and dim light of the area larvae settle predominantly on under surfaces. (5) In still water in the absence of light larvae settle predominantly on upper surfaces. (6) Under the conditions of current and light in the multiplate frames used to sample spatfall here, larvae settle mainly on upper surfaces. (7) Larvae tend to crawl up inclined surfaces before settling.

The results indicate that larval behaviour may be changed by small alterations of light intensity and current. The contradictory nature of surface angle preferences found by other workers for various species of Ostrea and Crassostrea may have been due to such small variations caused by the experimental techniques. It is possible that the settlement behaviour of all species of these genera is similar.     

Effect of maturity on carbon isotope ratios of oils and condensates

For modelling isotopic variations in oils it is convenient to differentiate the effects of oil generation ( 100–150°C) from the effects of oil to gas cracking ( 150–180°C). During generation, δ¹³C of kerogen may increase by up to 1% due to release of isotopically light oil and gas, although most kerogens show little or no chan δ¹³C of the generated oil increases by between 0 and 1% (av. 0.5%) due to mixing of isotopically heavy oil with an initial isotopically light unbound fraction, possibly of bacterial origin. The change occurs mostly over the first 20% of generation. During oil to gas cracking, kinetic isotope effects become important and the effect on δ¹³C of the remaining oil can be modelled as a Rayleigh process. δ¹³C increases by 1.5% by 50% cracking. Insufficient data are available to calibrate the effects at higher levels of cracking, and modelling these variations is hindered by a lack of understanding of the mechanism of pyrobitumen formation. However, increases greater than about 4% are unlikely to be observed. With increasing maturity, the low molecular weight fractions become isotopically heavy faster than the high molecular weight fractions. As a result, any separation of the low molecular weight fraction into a gas phase (“condensate formation”) will produce an isotopic difference between oil and condensate that depends on maturity. In the early stages of generation the condensate may be up to 1% lighter than the remaining oil. With increasing maturity, this difference at first decreases and then increases in the opposite sense. By half way through oil to gas cracking the condensate may be 1.5% heavier than the residual liquid. More subtle rearrangement reactions may result in small, but significant, changes to the shape of the isotope “type-curves” when different oil fractions are compared.