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1.
In an attempt to discover planetary eclipses, we observed the open cluster NGC 7086. On one night we observed the cluster and standard stars through the B and V filters, enabling us to make a colour-magnitude diagram. Plots of the differential magnitudes were inspected for variability, but no planetary eclipses were found. New variable stars were discovered and their light curves show some of them to be eclipsing binary stars. The location on the colour-magnitude diagram of some of the variable stars is consistent with cluster membership.  相似文献   
2.
To improve resolution of seismic-reflection profiles in continental slope water depths of 900 to 1500 m, a single hydrophone was towed about 150 m off the bottom to receive reflected signals from a surface-towed sparker sound source. That deep-towed hydrophone data show that valleys which appear V-shaped in records from a surface-towed hydrophone are flat-bottomed, and that subbottom reflections from an erosional unconformity can be much better resolved. The data produced by this technique are very hepful when used in conjunction with records from conventional surface-towed seismic-profiling equipment.  相似文献   
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To better image deformation structures within the inner accretionary wedge of the Nankai Trough, Japan, we apply common reflection angle migration to a legacy two-dimensional seismic data set acquired with a 6 km streamer cable. In this region, many seismic surveys have been conducted to study the seismogenic zone related to plate subduction. However, the details of the accreted sediments beneath the Kumano forearc basin are still unclear due to the poor quality of seismic images caused by multiple reflections, highly attenuated signals, and possibly complex geological structures. Generating common image gathers in the subsurface local angle domain rather than the surface offset domain is more advantageous for imaging geological structures that involve complex wave paths and poor illumination. By applying this method, previously unseen structures are revealed in the thick accreted sediments. The newly imaged geometric features of reflectors, such as the folds in the shallow part of the section and the deep reflectors with stepwise discontinuities, imply deformation structures with multiple thrust faults. The reflections within the deep accreted sediments (approximately 5 km) are mainly mapped to far angles (30°–50°) in the common reflection angles, which correspond to the recorded offset distances greater than 4.5 km. This result indicates that the far offset/angle information is critical to image the deformation structures at depth. The new depth image from the common reflection angle migration provides seismic evidence of multiple thrust faults and their relationship with the megathrust fault that is essential for understanding the structure and evolution of the Nankai Trough seismogenic zone.  相似文献   
5.
Jane Robb 《Geology Today》2013,29(2):63-67
Rising fees are forcing higher education institutions to think critically about what students are offered for their money. In geology courses there appears to be a lack of guidance for alternative careers in academia or industry, and even a lack of education about wider social, political and economic impacts of the discipline. It is possible to detect a lack of high‐impact geoscience among the popular science communication communities, such as online multidisciplinary blogging platforms. In order to enhance the student experience and the impact of geoscience on the wider public, universities need to look inwards at what they can do to help inspire and educate students to have broader career horizons and bigger public impacts through their research.  相似文献   
6.
Summary White micas from metamorphosed and hydrothermally-altered basaltic lavas, conglomerates, quartzites and shales in and around the Ventersdorp Contact Reef of the Witwatersrand Basin, South Africa, were dated by the K-Ar method to constrain post-depositional thermal and mineralization processes. The minerals were separated into various grain sizes between < 0.4 and 10m, and characterized in terms of composition, paragenetic sequence and texture, by XRD, SEM and TEM techniques. The K-Ar isochron of all white micas in the basaltic lavas suggests an age of 1994 ± 60 Ma, and that of the smaller mica particles (< 2m) in the quartzites defines a younger age of 1917 ± 66 Ma. This range is considered to reflect the timing of long-lived hydrothermal alteration in the Ventersdorp Contact Reef. The older age is slightly younger than the intrusion of the Bushveld Complex (2060–2054 Ma) and the Vredefort catastrophism (2020 Ma), which are well-documented events that were superimposed onto the Witwatersrand Basin. The younger age may be associated with the Eburnian orogenesis along the western edge of the Kaapvaal Craton resulting in continental-scale fluid migration and hydrothermal activity that extended throughout the Griqualand Basin and even into the Witwatersrand Basin. The K-Ar ages obtained here for the white mica fractions of the Ventersdorp Contact Reef in the Witwatersrand Basin confirm that the period between 2.0 and 1.9 Ga was significant, as far as alteration, and possibly also gold mobilization, was concerned.
K-Ar Datierung von Hellglimmern aus dem hentersdorp Contact Reef des Witwatersrand Beckens, Südafrika: die zeitliche Eingrenzung der nach der Sedimentablagerung erfolgten Alteration
Zusammenfassung Hellglimmer von metamorph und hydrothermal überprägtem Basalt, Konglomerat, Quarzit und Pelit aus dem Ventersdorp Contact Reef im Witwatersrand Becken, Südafrika, wurden mittels der K-Ar Methode datiert, um das Alter der postsedimentären thermischen Überprägung einzugrenzen. Mineralkörner wurden in einzelne Fraktionen zwischen < 0.4 und 10m separiert und auf deren Zusammensetzung, Paragenese und Textur mittels Röntgendiffraktometrie und Elektronenmikroskopie untersucht. Das Isochronenalter für alle Hellglimmerproben aus dem Metabasalt liegt bei 1994 ± 60 Ma, jenes für die Glimmer mit einer Korngröße < 2m im Quarzit bei 1917 ± 66 Ma. Diese Altersspanne wird als Ausdruck einer lang anhaltenden hydrothermalen Veränderung des Ventersdorp Contact Reef interpretiert. Das ältere Alter ist etwas jünger als die Intrusion des Bushveld Komplex (2060–2054 Ma) und die Vredefort Katastrophe (2020 Ma) - zwei gut dokumentierte Ereignisse, die das Witwatersrand Becken erfaßten. Das jüngere Alter könnte mit der eburnischen Orogenese entlang des Westrandes des Kaapvaal Kratons in Zusammenhang stehen, während der es zu Fluid Migration und hydrothermaler Aktivität quer über den Kontinent vom Griqualand Becken bis in das Witwatersrand Becken kam. Die neuen K-Ar Alter bestätigen somit, daß die Zeitspanne von 2.0–1.9 Ga wesentlich für die Alteration und möglicherweise auch für die Mobilisierung von Gold im Witwatersrand Becken war.
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7.
Summary Four metamorphic/hydrothermal fluid systems were identified in detailed microthermometric and spectroscopic investigations carried out on fluids trapped in late-stage quartz veins sampled throughout the Witwatersrand Basin. These include aqueous, H2O-CO2-rich, H2O-CH4-CO2-rich and CH4-N2-rich fluids. Early inclusion populations are dominated by H2O- and CO2-rich fluid systems. Cross-cutting these early fluid populations are trails of inclusions that contain CH4, C2H6, N2, H2 and H2S (vapour-rich inclusions). Fault-related quartz veins, in particular, are characterized by these later fluid types. A common feature of some of these later fluids is the presence of hydrocarbons and daughter crystals. A very late phase of aqueous fluids occurs in most samples as transgranular inclusion trails. P-V T-X considerations as well as chlorite geothermometry, mineral assemblages and burial conditions suggest entrapment temperatures of between 200°C and 400°C and locally up to 500°C. Fluid chemistry suggests that the post-depositional C-O-H fluids affecting the sediments have oxygen fugacities between Q-F-M and Ni-NiO in the range 300°C to 400°C. This accounts for the widespread preservation of detrital uraninite and gold remobilization along major fluid conduits.
Charakterisierung von post-sedimentären Fluiden im Witwatersrand-Becken
Zusammenfassung Vier verschiedene Arten von metamorphen/hydrothermalen Flüssigkeitseinschlüssen wurden im Zuge von detaillierten mikrothermometrischen und spektroskopischen Untersuchungen an Flüssigkeiten in Proben von spätgebildeten Quarzgängen aus dem Gesamtbereich des Witwatersrand-Beckens identifiziert. Bei diesen Flüssigkeiten konnten wässerige, H2O-CO2-reiche, H2O-CH4-CO2-reiche und CH4-N2-reiche Typen unterschieden werden. Bei frühgebildeten Einschlüssen dominieren H2O- und CO2-reiche Flüssigkeiten. Die frühen Einschlüsse kommen entlang verheilter Bruchflächen vor und werden von einer späteren, gasreichen Generation durchkreuzt, die CH4, C2H6, N2, H2, und H2S enthält. Insbesondere Quarzgänge, die an Verwerfungen gebunden sind, enthalten Flüssigkeitseinschlüsse des letzteren Typs. Einige dieser Flüssigkeiten haben die Anwesenheit von Tochterkristallen und hydrokarbonischer Komponenten gemeinsam. Eine sehr späte Generation von wäßrigen Flüssigkeiten kommt in den meisten Proben in der Form von trans-granularen Einschlussbahnen vor. Berücksichtigung von P-V-T-X Bedingungen und Chlorit-Thermometrie, von Mineralparagenesen und Überlagerungsmächtigkeit weisen auf Bildungstemperaturen zwischen 200 und 400 °C, lokal bis zu 500 °C. Die Zusammensetzungen der Flüssigkeiten deuten an, daß die spät-bis post-diagenetischen C-O-H Flüssigkeiten, die auf die Sedimente einwirkten, Sauerstoffugazitäten im Bereich zwischen Q-F-M und Ni-NiO, für Temperaturen von 300 bis 400 °C, hatten. Dies erkärt, warum detritischer Uraninit in weiten Bereichen des Beckens auftritt und warum Remobilisierung von Gold entlang von Zonen hoher Fluidwegsamkeit stattfinden konnte.
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The development of the post-nova light curve of V1500 Cyg inUBV andHβ, for 15 nights in September and October 1975 are presented. We confirm previous reports that superimposed on the steady decline of the light curve are small amplitude cyclic variations. The times of maxima and minima are determined. These together with other published values yield the following ephemerides from JD 2 442 661 to JD 2 442 674: $$\begin{gathered} {\text{From}} 17 {\text{points:}} {\text{JD}}_{ \odot \min } = 2 442 661.4881 + 0_{^. }^{\text{d}} 140 91{\text{n}} \hfill \\ \pm 0.0027 \pm 0.000 05 \hfill \\ {\text{From}} 15 {\text{points:}} {\text{JD}}_{ \odot \max } = 2 442 661.5480 + 0_{^. }^{\text{d}} 140 89{\text{n}} \hfill \\ \pm 0.0046 \pm 0.0001 \hfill \\ \end{gathered} $$ with standard errors of the fits of ±0 . d 0052 for the minima and ±0 . d 0091 for the maxima. Assuming V1500 Cyg is similar to novae in M31, we foundr=750 pc and a pre-nova absolute photographic magnitude greater than 9.68.  相似文献   
10.
Contamination of groundwater with chlorinated ethenes is common and represents a threat to drinking water sources. Standard anaerobic bioremediation methods for the highly chlorinated ethenes PCE and TCE are not always effective in promoting complete degradation. In these cases, the target contaminants are degraded to the daughter products DCE and/or vinyl chloride. This creates an additional health risk, as vinyl chloride is even more toxic and carcinogenic than its precursors. New treatment modalities are needed to deal with this widespread environmental problem. We describe successful bioremediation of a large, migrating, dilute vinyl chloride plume in Massachusetts with an aerobic biostimulation treatment approach utilizing both oxygen and ethene. Initial microcosm studies showed that adding ethene under aerobic conditions stimulated the rapid degradation of VC in site groundwater. Deployment of a full‐scale treatment system resulted in plume migration cutoff and nearly complete elimination of above‐standard VC concentrations.  相似文献   
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