Petrology, geochemistry, and U-Pb (zircon) age of the quartz-feldspar porphyry dyke at the Lake George antimony mine, New Brunswick: implications for origin, emplacement process, and mineralization

A steeply west-dipping, north-northwest-trending, biotite-bearing quartz-feldspar porphyry dyke is associated with the Lake George granodiorite, a cupola of the Pokiok Batholith. These Early Devonian intrusions are spatially and temporally related to W-Mo-Au and Sb-Au mineralization in the area. The porphyry dyke yielded an age of 420.8 +5.9/-4.0 Ma (U-Pb zircon) and is inferred to be coeval with or slightly older than the Lake George granodiorite (412 +5/-4 Ma, U-Pb zircon). The variably altered dyke contains subhedral to anhedral (rounded) quartz, plagioclase, and orthoclase phenocrysts (0.5 to 30 mm; 30 to 60 vol. %), and numerous angular to subrounded xenoliths of altered intrusion carapace and quenched dyke rocks, as well as local Kingsclear Formation metasedimentary rocks. The dyke is similar to the Lake George granodiorite in phenocryst population, volcanic arc (I-type) affinity, average Zr (157 ppm), TiO2 (0.54 %), La/Yb ratio (13), and REE (129 ppm). The average Au content is lower in the dyke (20 ppb) than in the granodiorite (32 ppb), the abundance of gold is related to minor magmatic hydrothermal chalcopyrite and pyrrhotite (< 2 %). Based on textural evidence, including autobrecciation, coupled with rheological and thermal modeling calculations for the 5 m-wide dyke, it is suggested that fluidization (vapour exsolution) of the magma was key to its rapid emplacement as a quenched glass-gas mixture (tuffisite). The S abundance and S isotopic signature of the dyke, relative to Au and Cu abundance, support reduced I-type magmatic volatiles involved in dyke emplacement and cogenetic autometasomatic alteration. RÉSUMÉ Un dyke de porphyre quartzo-feldspathique renfermant de la biotite, orienté vers le nord-nord-ouest et s’inclinant abruptement vers l’ouest, est associé à la granodiorite du lac George, une coupole du magmatisme du batholite de Pokiok. Ces intrusions régionales du Dévonien précoce sont spatialement et temporellement apparentées à une minéralisation de W-Mo-Au et de Sb-Au dans le secteur. Le dyke de porphyre a accusé un âge de 420,8 +5,9/-4,0 Ma (U-Pb sur zircon) et on le suppose du même âge ou légèrement plus âgé que la granodiorite du lac George (412 +5/-4 Ma, U-Pb sur zircon). Le dyke altéré de façon variable abrite des phénocristaux hypautomorphes à allotriomorphes (arrondis) de quartz, de plagioclase et d’orthoclase (0,5 à 30 mm, 30 à 60 % en vol.) ainsi que de nombreux xénolites angulaires à subsphérique d’une carapace d’intrusion altérée et de roches de dykes noyées, en plus de roches métasédimentaires locales de la Formation de Kingsclear. Le dyke s’avère analogue à la granodiorite du lac George du point de vue de la population de phénocristaux, de l’affinité avec l’arc insulaire (de type intrusif), de la concentration moyenne de Zr (157 ppm), du TiO2 (0,54 %), du ratio de La/Yb (13) et des ÉTR (129 ppm). La teneur moyenne en Au est plus faible dans le dyke (20 parties par milliard) que dans la granodiorite (32 parties par milliard); son abondance est apparentée à la présence restreinte de chalcopyrite et de pyrrhotite hydrothermales magmatiques (< 2 %). Selon les indices texturaux, notamment l’autobréchification, conjugués à des calculs de modélisation rhéologique et thermale du dyke (5 m), on peut supposer que la fluidisation (exsolution à l’état de vapeur) du magma a contribué à sa mise en place rapide sous forme d’un mélange de verre-gaz (tuffisite) noyé. L’abondance de S et la signature isotopique du S du dyke, comparativement à l’abondance d’Au et de Cu, appuient la participation réduite d’éléments volatils magmatiques de type intrusif à la mise en place du dyke et à l’altération autométasomatique cogénétique. [Traduit par la rédaction

Analyses of Dental Pulp in Restored Teeth

Restored teeth were extracted from test animals at four time intervals (1 hour, 1 day, 1 week, and 3 months) following amalgam insertion. Extracted teeth were frozen in liquid nitrogen, cryo-fractured so as to expose the pulps and then freeze-dried. Pulps were analyzed for mercury content by energy dispersive spectrometry (EDS) and atomic absorption spectrophotometry (AAS). Mercury levels appeared below the detection limits of EDS but could be detected by AAS which showed the highest readings seven days after amalgam insertion

Chemostratigraphy and depositional environment of an Ordovician sedimentary section across the Miramichi Group - Tetagouche Group contact, northeastern New Brunswick

A thick section of Ordovician sedimentary rocks underlies and overlies felsic to mafic volcanic rocks of the Tetagouche Group, Bathurst Mining Camp. The dark grey quartzose slates and siltstones of the Patrick Brook Formation (Miramichi Group) occur below the volcanic rocks, whereas the dark grey to black slates and siltstones of the Boucher Brook Formation (Tetagouche Group) are intercalated with the volcanic rocks and overlie the sequence. The Miramichi-Tctagouche contact represents the interpreted Gander-Dunnage boundary in northeastern New Brunswick. Distinguishing between these two simitar formations is important for stratigraphic and geo-tectonic interpretations of the Bathurst Mining Camp and for exploration in these sequences. The geochemical composition of a semi-con form able section of rocks from the Boucher Brook (Middle to Late? Ordovician) and Patrick Brook (Early to Middle Ordovician) formations was determined to identify geochemical chemostratigraphic discriminants, as well as to determine the depositional environment in which these were deposited. The high AI2O3 and distinctly higher high-field-strength elements (LREE, Th, HREE, and Y) in the Patrick Brook rocks are characteristic of mature sedimentary rocks and indicate intense chemical weathering (tropical environment) in the source regions, which is consistent with their compositional similarity to Avalon-derived shales analogous to Gander Zone sedimentary rocks. The Boucher Brook slates and siltstones are immature sedimentary rocks based on the preservation of albite and the less coherent trace-element systematics to phyllosilicate indices (AI2O3 and K2O). The Boucher Brook Formation is probably derived from the associated volcanic rocks. The higher Mn and Fe and positive Ce/Ce* anomaly in some Boucher Brook Formation compared to the Patrick Brook rocks indicate that the Boucher Brook rocks in this section were deposited in a transitional anoxic/ oxic environment. The Patrick Brook rocks that immediately precede felsic volcanism and formation of massive sulphide deposits are highly reduced based on C and S contents, which is consistent with the sulphur isotope data. Moderately heavy &#x3B4;34S values are indicative of SO42- reduction to H2S under anoxic conditions, which is significant in the formation and preservation of massive sulphides in the basal Tetagouche sequence. R&#xC9;SUM&#xC9; Une section &#xE9;paisse de roches s&#xE9;dimentaires de l’Ordovicien est sus-jacente ct sous-jacente &#xE0; des roches volcanomafiques &#xE0; volcanofelsiques du groupe de Tetagouche, dans le Camp minier de Bathurst. Des siltstones et des schistes quartzeux gris fonc&#xE9; de la Formation de Patrick Brook (groupe de Miramichi) sont pr&#xE9;sents au-dessous des roches volcaniques, tandis que des schistes et des siltstones gris fonc&#xE9; &#xE0; noirs de la formation de Boucher Brook (groupe de Tetagouche) sont intercales dans les roches volcaniques et recouvrent la s&#xE9;quence. La surface de contact de Miramichi-Tetagouche repr&#xE9;sente ce qu'on interpr&#xE8;ts comme la limite de Gander-Dunnage dans le nord-est du Nouveau-Brunswick. Il est important d'&#xE9;tablir une distinction entre ces deux formations semblables pour les interpr&#xE9;tations stratigraphiques du Camp minier de Bathurst et pour l'exploration dans ces s&#xE9;quences. On a d&#xE9;termine la composition g&#xE9;ochimique d'une section semi-concordante de roches de Boucher Brook (Ordovicien moyen &#xE0; tardif?) et de Patrick Brook (Ordovicien inf&#xE9;rieur &#xE0; moyen) afin de rep&#xE9;rer les discriminants chimiostratigraphiques g&#xE9;ochimiques ainsi que pour d&#xE9;finir le milieu s&#xE9;dimentaire dans lequel ceux-ci ont &#xE9;t&#xE9; deposes. La quantit&#xE9; prononc&#xE9;e d'Al2O3 et la pr&#xE9;sence distinctement sup&#xE9;rieure d'&#xE9;l&#xE9;ments d'intensit&#xE9; de champ &#xE9;lev&#xE9;e (&#xE9;l&#xE9;ments de terres rares l&#xE9;gers, Th, &#xE9;l&#xE9;ments de terres rares lourds et Y) dans les roches de Patrick Brook constituent des traits caract&#xE9;rstiques de roches s&#xE9;dimentaires matures; el les t&#xE9;moignent d'une alt&#xE9;ration climatique chimique intense (milieu tropical) dans les regions d'origine, ce qui est compatible avec la similarit&#xE9; de leur composition avec les schistes en provenance d'Avalon analogues aux roches s&#xE9;dimentaires de la zone de Gander. Les schistes et les siltstones de Boucher Brook sont des roches s&#xE9;dimentaires immatures bas&#xE9;es sur la conservation d'albite et la corr&#xE9;lation d'&#xE9;l&#xE9;ments traces moins coh&#xE9;rents avec les indices de phyllosilicates (AI2O3). La Formation de Boucher Brook provient probabtement de roches volcaniques connexes. La proportion sup&#xE9;rieure de Mn et de Fe et l’anomalie positive de Ce/Ce* dans certaines parties de la Formation de Boucher Brook r&#xE9;v&#xE8;lcnt que les roches de Boucher Brook de cette section ont &#xE9;t&#xE9; d&#xE9;pos&#xE9;es dans un milieu anoxique / oxique de transition. Les roches de Patrick Brook qui ont imm&#xE9;diatement pr&#xE9;ced&#xE9; le volcanisme felsique et la formation de gitcs de sulfures massifs ont, &#xE0; en juger par Icur teneur en C et en S, subi une r&#xE9;duction importante, ce qui correspond aux donn&#xE9;es isotopiques relatives au soufre. Les valeurs moyennement prononc&#xE9;es de &#x3B4;34S temoignent d'une r&#xE9;duction du SO42- en H2S dans des conditions anoxiques, un ph&#xE9;nom&#xE8;ne d&#xE9;terminant dans la formation et la conservation des sulfures massifs dans la s&#xE9;quence basale de Tetagouche. [Traduit par la r&#xE9;daction

Specific contribution of different phospholipid surfaces to the activation of prothrombin by the fully assembled prothrombinase

This paper addresses, in thermodynamic and kinetic terms, the reasons for the acidic lipid specificity of the human prothrombinase complex. We obtained, from the measured lipid titrations of the initial rates of prothrombin activation, the empirical binding constants for prothrombinase assembly on different membranes. These favored assembly on phosphatidylserine (PS)- as opposed to phosphatidylglycerol (PG)-containing membranes. In addition, we have used full time courses of prothrombin activation, in conjunction with a calculation of the equilibrium distribution of factor Xa between four enzymatic forms, to obtain the intrinsic kinetic constants of the prothrombinase assembled on PS- or PG-containing membranes. The resulting values of kcat, Km, and kcat/Km increased as acidic lipid content increased, and kcat/Km reached a plateau at 12 mol % PS and 50 mol % PG. Using the measured assembly and kinetic constants, the observed shapes of the phospholipid titration curves of human prothrombin activation were interpreted. We conclude that the difference in activity of prothrombinase assembled on PS- versus PG-containing membranes results both from the different binding properties of factors Xa and Va to these surfaces and from the different intrinsic activities of the prothrombinase when assembled on different membranes

Statistical Similarities Between WSA‐ENLIL+Cone Model and MAVEN in Situ Observations From November 2014 to March 2016

Normal solar wind flows and intense solar transient events interact directly with the upper Martian atmosphere due to the absence of an intrinsic global planetary magnetic field. Since the launch of the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission, there are now new means to directly observe solar wind parameters at the planet’s orbital location for limited time spans. Due to MAVEN’s highly elliptical orbit, in situ measurements cannot be taken while MAVEN is inside Mars’ magnetosheath. To model solar wind conditions during these atmospheric and magnetospheric passages, this research project utilized the solar wind forecasting capabilities of the WSA‐ENLIL+Cone model. The model was used to simulate solar wind parameters that included magnetic field magnitude, plasma particle density, dynamic pressure, proton temperature, and velocity during a four Carrington rotation‐long segment. An additional simulation that lasted 18 Carrington rotations was then conducted. The precision of each simulation was examined for intervals when MAVEN was in the upstream solar wind, that is, with no exospheric or magnetospheric phenomena altering in situ measurements. It was determined that generalized, extensive simulations have comparable prediction capabilities as shorter, more comprehensive simulations. Generally, this study aimed to quantify the loss of detail in long‐term simulations and to determine if extended simulations can provide accurate, continuous upstream solar wind conditions when there is a lack of in situ measurements.Plain Language SummaryIf we ever have a manned mission to Mars, one of the numerous concerns would be space weather conditions and their effects on spacecraft in flight. One particular element of space weather that we like to focus on is solar wind: plasma that is continuously emitted from the Sun. Solar wind can effect communication between Earth and spacecraft, GPS services, and other vital elements of space travel. We therefore want a good understanding of space weather and want to forecast conditions before ever traveling there. Currently, there are not always means to directly measure solar wind, so we rely on numerical models. In this study, we used the model called WSA‐ENLIL+Cone to compare its solar wind measurements and one of our spacecraft orbiting Mars to see how well it did and to see if we can rely on it for solar wind forecasts. As it turns out, the model can be used for forecasting baseline values of different solar wind parameters, for example, temperature, even with limited information. We show in this study that the WSA‐ENLIL+Cone model allows us to forecast solar wind conditions and helps us to understand what is going on at that seemingly barren planet.Key PointsGeneralized, extensive WEC model simulations provide analogous confidence levels and results as detailed, relatively short simulationsWSA‐ENLIL+Cone model succeeds at predicting fast solar wind radial velocityPeer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/142959/1/swe20547.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/142959/2/swe20547_am.pd

Evidence for Asphericity in the Type IIn Supernova 1998S

We present optical spectropolarimetry obtained at the Keck-II 10-m telescope on 1998 March 7 UT along with total flux spectra spanning the first 494 days after discovery (1998 March 2 UT) of the peculiar type IIn supernova (SN) 1998S. The SN is found to exhibit a high degree of linear polarization, implying significant asphericity for its continuum-scattering environment. Prior to removal of the interstellar polarization, the polarization spectrum is characterized by a flat continuum (at p ~ 2%) with distinct changes in polarization associated with both the broad (FWZI >= 20,000 km/s) and narrow (unresolved, FWHM < 300 km/s) line emission seen in the total flux spectrum. When analyzed in terms of a polarized continuum with unpolarized broad-line recombination emission, an intrinsic continuum polarization of p ~ 3% results (the highest yet found for a SN), suggesting a global asphericity of >= 45% from the oblate, electron-scattering dominated models of Hoflich (1991). The smooth, blue continuum evident at early times is shown to be inconsistent with a reddened, single-temperature blackbody, instead having a color temperature that increases with decreasing wavelength. Broad emission-line profiles with distinct blue and red peaks are seen in the total flux spectra at later times, perhaps suggesting a disk-like or ring-like morphology for the dense (n_e ~ 10^7 cm^{-3}) circumstellar medium. Implications of the circumstellar scattering environment for the spectropolarimetry are discussed, as are the effects of uncertain removal of interstellar polarization.Comment: 25 pages + 2 tables + 14 figures, Submitted to The Astrophysical Journa

Quantitative analysis of cell types during growth and morphogenesis in Hydra

Tissue maceration was used to determine the absolute number and the distribution of cell types in Hydra. It was shown that the total number of cells per animal as well as the distribution of cells vary depending on temperature, feeding conditions, and state of growth. During head and foot regeneration and during budding the first detectable change in the cell distribution is an increase in the number of nerve cells at the site of morphogenesis. These results and the finding that nerve cells are most concentrated in the head region, diminishing in density down the body column, are discussed in relation to tissue polarity

Ordered and disordered phospholipid domains coexist in membranes containing the calcium pump protein of sarcoplasmic reticulum.

Data are presented that lead to an alternative model for the organization and molecular dynamics of lipid molecules near the Ca2+-stimulated, Mg2+-dependent adenosinetriphosphatase (Ca2+-ATPase; ATP phosphohydrolase, EC 3.6.1.3) of sarcoplasmic reticulum. Measurements of the steady-state fluorescence anisotropy of 1,6-diphenyl-1,3,5-hexatriene in progressively delipidated sarcoplasmic reticulum membranes have been quantitatively interpreted in terms of a layer of lipid of high anisotropy (the lipid annulus) coexisting with lipid layers of very low anisotropy. In addition, the Ca2+-ATPase has been reconstituted into pure 1,2-dipentadecanoyl 3-sn-phosphatidylcholine membranes over a range of lipid-to-protein ratios. High-sensitivity differential scanning calorimetry has demonstrated that roughly 30 lipid molecules per Ca2+-ATPase molecule (annular lipids) fail to undergo a calorimetrically detectable phase transition in the temperature range 4-44 degrees C. Roughly 100 lipid molecules beyond the annulus undergo a detectable phase transition at a temperature below the phase transition of pure lipid and with an enthalpy change [4.2 kcal/mol (1 kcal = 4.18 kJ)] about half that observed for pure lipid vesicles (7.7-7.8 kcal/mol). We propose that both the fluorometric and calorimetric data are consistent with a model in which a motionally inhibited lipid annulus is surrounded by a more extensive region of disrupted lipid packing order, which we have called the secondary lipid domain