In memory of L. V. Anfimov

Chronicle

In memory of L. V. Anfimov     

The 80th Anniversary of V.N. Kholodov

Chronicle

The 80th Anniversary of V.N. Kholodov     

REVIEW OF THALLIUM,ITS GEOCHEMISTRY,MINERALOGY, PRINCIPAL GENETIC TYPES OF DEPOSITS,AND GEOCHEMICAL PROVINCES BY V.V. IVANOV,V.YU. VOLGIN,A.A. KRASNOV AND N.V. LIZUNOV

This book review takes the authors to task for omitting numerous references when they wrote this first comprehensive work on thallium. Among the omissions noted are; 1) the extreme toxicity of thallium; 2) the occurrence of thallium in various minerals:

REVIEW OF THALLIUM, ITS GEOCHEMISTRY, MINERALOGY, PRINCIPAL GENETIC TYPES OF DEPOSITS, AND GEOCHEMICAL PROVINCES BY V.V. IVANOV, V.YU. VOLGIN, A.A. KRASNOV AND N.V. LIZUNOV

All authors

V. V. Mogarovskiy

https://doi.org/10.1080/00206816409473950

Published online:

20 September 2010

Table     

Physical parameters of the eclipsing binary V798 Cep

The first high-accuracy CCD UBV RI(RI)_C light curves for the recently discovered eclipsing binary V798 Cep (P = 16 ^d .08, V = 11 ^m . 8) are presented; this star is included in our program of eclipsing systems with considerable eccentricities. A photometric solution for the light curves and physical characteristics of the component stars are derived. The orbital eccentricity is quite high, e = 0.437. The longitude of periastron is close to 180°, making studies of the apsidal motion difficult. V798 Cep may be a hierarchical system.     

<Emphasis Type="Bold">Paleoproterozoic Boninite-Like Rocks in an Intracratonic Setting from Northern Bastar Craton,Central India</Emphasis> by D.V. Subba Rao,V. Balaram,K. Naga Raju and D.N. Sridhar. Jour. Geol. Soc. India,v.72, 2008, pp.373–380

Discussion

Paleoproterozoic Boninite-Like Rocks in an Intracratonic Setting from Northern Bastar Craton, Central India by D.V. Subba Rao, V. Balaram, K. Naga Raju and D.N. Sridhar. Jour. Geol. Soc. India, v.72, 2008, pp.373–380     

Symposium on the Geomorphology of Southern Africa

Reports

International/National Conference on Advances in Ground-Water Hydrology, dedicated to the memory of Dr. C. V. Theis, will be held Nov. 16–18, 1988 Tampa, Florida, USA     

Unusual Photometric Activity of the Weak-line T Tauti Star V715 Per

The results of many-year photometric observations of the weak-line T Tauri star V715 Per in the optical (V RI) and infrared (JHK) photometric bands are presented. The period of the star’s lowamplitude brightness variations in the V RI bands detected earlier, 5.23d, is confirmed. This period persists during the entire 14-year time interval of the observations, but its amplitude varies with time. The same period was found in the variations of JHK infrared fluxes, with the brightness variations in the two ranges being almost synchronous. The most probable origin of these variations is periodic eclipses of the star by its own disk, perturbed by its interaction with the magnetosphere (AA Tau-type variations). In addition to the periodic brightness variations, the star also displayed sporadic Algol-like minima characteristic of UX Ori stars during several years (2005–2011). The amplitude of these variations increasedmonotonically, reaching approximately 1^m in the V band by the end of 2010, after which the deep fadings ended. During this entire time interval, the amplitude of the periodic variations was observed to decrease. After 2011, the periodic component began to become stronger again. These changes of the photometric activity of V715 Per can be explained by an increasing rate of gas accretion onto the star, decreasing the radius of warped regions of the disk and leading to accompanying Algol-like fadings. This model assumes a low inclination of the circumstellar disk in V715 Per to the line of sight.     

Comment on “Hydrolysis of neptunium(V) at variable temperatures (10-85 °C)” by L. Rao, T.G. Srinivasan, A.Yu. Garnov, P. Zanonato, P. Di Bernardo, and A. Bismondo

In a recent study [Rao, L., Srinivasan, T.G., Garnov, A.Yu., Zanonato, P., Di Bernardo, P., Bismondo, A., 2004. Hydrolysis of neptunium(V) at variable temperatures (10-85 °C). Geochim. Cosmochim. Acta68, 4821-4830.] the hydrolysis of Np(V) was investigated at 10-85 °C by absorption spectroscopy, potentiometry, and microcalorimetry along the titration of Np(V) solutions with tetramethylammonium hydroxide up to pH 10. However, there is strong evidence that the precautions to avoid competing reactions with carbonate were not sufficient and that the measured effects are not caused by the formation of Np(V) hydroxide complexes but primarily by the formation of Np(V) carbonate complexes. The reported equilibrium constants, enthalpies, entropies, and heat capacities for the complexes NpO₂OH(aq) and are severely in error and must not be used for the geochemical modeling of neptunium. If the hydrolysis constants reported by Rao et al. [Rao, L., Srinivasan, T.G., Garnov, A.Yu., Zanonato, P., Di Bernardo, P., Bismondo, A., 2004. Hydrolysis of neptunium(V) at variable temperatures (10-85 °C). Geochim. Cosmochim. Acta68, 4821-4830] are used to calculate neptunium solubilities in alkaline solutions relevant for nuclear waste repositories, the Np(V) concentrations are overestimated by orders of magnitude.     

A brief summary of Dr. G. V. Rao’s research interests

A brief summary of Dr. G. V. Rao's research interests is presented. Many of his earlier studies were in conjunction with the summer Monsoon Experiment of 1979 (MONEX-79). These included: 1) the structure of the Somali jet based on aerial observations; 2) sea-level air trajectories over the equatorial Indian Ocean; 3) structural features of the east African low-level flow; 4) effects of Indian Ocean surface temperature anomaly patterns on the summer monsoon circulations; 5) structures of the monsoon low-level flow over the Arabian Sea; 6) characteristics and momentum-flux budgets of the Arabian Sea convective bands; and 7) evaporation and precipitation over the Arabian Sea during the monsoon seasons. Dr. Rao's research efforts in recent years had focused on case studies of mesocyclones spawned by tropical cyclones (TCs) in Florida using Doppler radar data and a mesoscale numerical model. These included: 1) research on tornadic mesocyclones spawned by TC Earl in 1998; 2) documentation of subtle differences between tornadic and non-tornadic mesocyclones in TC Floyd in 1999; and 3) numerical simulation of the tornadic environment observed in peninsular Florida during TC Earl in 1998. Preliminary findings show that the supercells' cold pools interacted with an existing boundary resulting in increased baroclinicity and horizontal vorticity, and a maximization of the tornado production potential by the updrafts. The model successfully simulated the mesoscale features of the mesocyclones and the tornadic environment observed during TC Earl. A 24 h simulation of accumulated rainfall within the inner domain agreed well with the observed precipitation pattern over the region.     

Isotopic datings of reddish granitoids in southern Värmland,southwestern Sweden

Three reddish granites from the Gneiss Complex of south-western Sweden have been dated with the U-Pb and one of them also with the Rb-Sr method. The Gneiss Complex consists of two mega-units separated by a tectonic discontinuity. The two granites from the western mega-unit (»the Western Gneiss Segment«) yield zircon upper-intercept ages of 1552 _–36 ⁺³⁸ and 1499 _–36 ⁺³⁶ Ma (2). These ages are minimum estimates of the intrusion ages, but the difference between the obtained and the true age is probably small. This assumption is based on studies of the morphology and internal structures of the zircons and also on air abrasion experiments.The third granite is located in the eastern mega-unit (the »Eastern Gneiss Segment«) and forms a number of small massifs, 50 m in diameter. The U-Pb and Rb-Sr ages agree within the limits of the errors — 1140 _–52 ⁺⁵⁴ Ma (upper intercept) and 1104 ± 100 Ma, respectively — but the obtained age is nevertheless dubious. Thin-section studies reveal that the zircons are heterogeneous with different types of material making up the inner and outer parts. Electron-microscopic studies as well as air abrasion and leaching experiments were performed to establish possible differences in age and chemistry between the inner and outer parts. The central parts are made up of almost pure ZrSiO₄ whereas the outer parts are layered with alternating pure ZrSiO₄ layers and layers rich in trace elements. The leaching and air abrasion data do not indicate any age difference between the inner and outer parts. This supports the validity of the upper-intercept age as an intrusion age.The Rb-Sr age is questionable since the obtained initial⁸⁷Sr/⁸⁶Sr ratio is as low as 0.7027. This cannot possibly be true for a felsic, late Proterozoic granite. A plausible explanation could be a rotation of the isochron due to migration of Rb and Sr during a low-grade event. This event is also responsible for the alteration of the biotites and plagioclases.These data provide additional evidence for extensive ensialic magmatism in the period succeeding the lithosphere-forming event.

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Zusammenfassung Drei rötliche Granite aus dem Südwestschwedischen Gneiskomplex sind mit der U-Pb Methode und einer davon zusätzlich mit der Rb-Sr Methode datiert worden. Der Gneiskomplex besteht aus zwei Haupteinheiten, die tektonisch voneinander getrennt sind. Zwei Granite aus der westlichen Haupteinheit (dem sogenannten »Western Gneiss Segment«) ergeben obere Schnittpunktsalter der Zirkone von 1552 _–36 ⁺³⁸ bzw. 1499 _–36 ⁺³⁶ Ma (2). Diese Alter stellen Minimumalter für die Instrusionen dar, die nur geringfügig jünger sind als die wahren Instrusionsaltern. Diese Vermutung stützt sich auf Untersuchungen der Morphologie und der internen Struktur der Zirkone sowie auf Experimente mit Hilfe der Luftabriebstechnik (air abrasion technique).Der dritte Granit stammt aus der östlichen Haupteinheit (dem sogenannten »Eastern Gneiss Segment«), in der er kleine Körper von etwa 50 m Durchmesser bildet. Die U-Pb und Rb-Sr Alter von 1140 _–52 ⁺⁵⁴ Ma (oberer Schnittpunkt), bzw. 1104 ± 100 Ma stimmen innerhalb des Fehlers überein. Trotzdem ist dieses Alter fragwürdig. Dünnschliffuntersuchungen zeigen, da\ die Zirkone heterogen sind, und da\ Rand und Kern unterschiedlich zusammengesetzt sind. Um Unterschiede in Alter und Chemismus zwischen Rand und Kern festzustellen, wurden Untersuchungen mit dem Elektronenmikroskop, Luftabriebsexperimente und Anätzexperimente durchgeführt. Die Kerne bestehen fast aus reinem ZrSiO₄, wogegen die äu\eren Ränder aus Wechsellagerungen von reinem ZrSiO₄ und Lagen mit hohem Spurenelementgehalt bestehen.Die Anätzversuche und die Luftabriebsexperimente brachten keinen Altersunterschied zwischen Rand und Kern. Diese Tatsachen sprechen dafür, da\ das obere Schnittpunktsalter dem Instrusionsalter entspricht.Das Rb-Sr Alter ist fragwürdig, zumal das⁸⁷Sr/⁸⁶Sr-Initialverhältnis einen sehr niedrigen Wert von 0,7027 aufweist, der für einen spätproterozoischen Granit viel zu niedrig ist. Eine mögliche Erklärung ist die Rotation der Isochrone wegen einer Migration von Rb und Sr während eines Ereignisses bei niedriger Temperatur, ein Ereignis, das auch für die Umwandlung von Biotit und Plagioklas verantwortlich zu sein scheint. Die oben aufgeführten Daten geben zusätzliche Hinweise für einen sialischen Magmatismus im Zeitraum des fortschreitenden Ereignisses der Bildung der Lithosphäre.

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Résumé Trois granites rougeâtres provenant du complexe gneissique du sud-ouest de la Suède ont été datés par la méthode U-Pb et, pour l'un d'entre eux, également par la méthode Rb-Sr. Le complexe gneissique consiste en deux grandes unités séparées par une discontinuité tectonique. Les zircons de deux granites provenant de l'unité occidentale (»Western Gneiss Segment«) fournissent des âges (intersection supérieure) de 1552 _–36 ⁺³⁸ et 1499 _–36 ⁺³⁶ Ma (2). Ces âges constituent des estimations minimales des âges d'intrusion, la différence entre l'âge mesuré et l'âge véritable étant probablement minime. Cette supposition se base sur l'étude de la morphologie et des structures internes des zircons, ainsi que sur des expériences d'abrasion à l'air.Le troisième granite est situé dans l'unité orientale (»Eastern Gneiss Segment«) et se présente en plusieurs massifs d'une cinquantaine de mètres de diamètre. Les âges U-Pb et Rb-Sr coÏncident dans les limites des erreurs (1140 _–52 ⁺⁵⁴ (point d'intersection supérieur) et 1104±100 Ma) l'âge obtenu étant néanmoins incertain. L'étude en coupes minces montre que les zircons sont hétérogènes, leurs parties centrales et périphériques présentant des constitutions différentes. Des examens au microscope électronique, ainsi que des essais d'abrasion à l'air et de corrosion à l'acide ont eté effectués afin de mettre en évidence des différences éventuelles d'âge et de composition chimique entre les parties contrales et périphériques. Tandis que les parties centrales consistent en ZrSiO₄ pratiquement pur, les parties extérieures se composent de couches de ZrSiO₄ pur alternant avec des couches contenant de multiples éléments en traces. Les données obtenues sur les grains corrodés à l'acide ou soumis à une abrasion à l'air n'indiquent cependant pas de différence d'âge entre les parties centrales et périphériques. Ceci confirme la validité de l'âge obtenu (point d'intersection supérieur) comme âge d'intrusion.L'âge Rb-Sr est douteux, étant donné que le rapport initial⁸⁷Sr/⁸⁶Sr n'est que de 0,7027, valeur improbable pour un granite felsique du ProtérozoÏque supérieur. Il paraÎt raisonnable de supposer une rotation de l'isochrone, due à une migration de Rb et Sr durant un événement à basse température. Cet événement serait également responsable de l'altération des biotites et des plagioclases. Ces données fournissent un argument supplémentaire en faveur d'un magmatisme ensialique pendant la période qui suit la formation de la lithosphère.

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- U/Pb, Rb/Sr. , . — . . Western Gneiss Segments — 1552 _–36 ⁺³⁸ 1499 _–36 ⁺³⁶ (2). . , air abrasion technique. — Eastern Gneiss Segments —, 50 . U/Pb 1140 _–52 ⁺⁵⁴ Ma ( ), Rb/Sr - 1104 ± 100 ; , . . , . , : , air abrasion technique . ZrSiO₄, ZrSiO₄, . air abrasion technique . , ., Rb/Sr, , ⁸⁷Sr/⁸⁶Sr (0,7027), . . - . — , , , . , .

     

In memory of I. K. Korolyuk

Chronicle

In memory of I. K. Korolyuk     

The centenary of G. F. Krasheninnikov

Chronicle

The centenary of G. F. Krasheninnikov     

In memory of M. A. Rateev

Chronicle

In memory of M. A. Rateev     

In memory of N.G. Brodskaya

Chronicle

In memory of N.G. Brodskaya     

<Emphasis Type="Bold">Synplutonic Mafic Dykes from Late Archaean Granitoids in the Eastern Dharwar Craton,Southern India</Emphasis> by M. Jayananda,T. Miyazaki,R.V. Gireesh,N. Mahesha and T. Kano. Jour. Geol. Soc. India,v.73, 2009, pp.117–130

Discussion

Synplutonic Mafic Dykes from Late Archaean Granitoids in the Eastern Dharwar Craton, Southern India by M. Jayananda, T. Miyazaki, R.V. Gireesh, N. Mahesha and T. Kano. Jour. Geol. Soc. India, v.73, 2009, pp.117–130     

V.V. Menner and activity of Interdepartmental Stratigraphic Committee and International Commission on Stratigraphy

Extraordinary significance of V.V. Menner activity for effective work of the Interdepartmental Stratigraphic Committee aimed at organization of stratigraphic survey and enhancement of stratigraphic research in the country is demonstrated. As chairperson of the International Commission on Stratigraphy, he made an outstanding contribution to its structuring and transformation into fruitful international institution supervising works on all subdivisions of the International Stratigraphic Scale.     

The 80th Birthday of B.M. Mikhailov

Chronicles

The 80th Birthday of B.M. Mikhailov     

Peculiarities and variations in the optical spectrum of the post-AGB star V448 Lac = IRAS 22223+4327

Multi-epoch observations with high spectral resolution acquired in 1998–2008 are used to study the time behavior of the spectral-line profiles and velocity fields in the atmosphere and circumstellar shell of the post-AGB star V448 Lac. Asymmetry of the profiles of the strongest absorption lines with lower-level excitation potentials χ _low < 1 eV and time variations of these profiles have been detected, most prominently the profiles of the resonance lines of BaII, YII, LaII, SiII. The peculiarities of these profiles can be explained using a superposition of stellar absorption line and shell emission lines. Emission in the (0; 1) 5635 Å Swan system band of the C₂ molecule has been detected in the spectrum of V448 Lac for the first time. The core of the Hα line displays radial-velocity variations with an amplitude of ΔV _r ≈ 8 km/s. Radial-velocity variations displayed by weak metallic lines with lower amplitudes, ΔV _r ≈ 1–2 km/s, may be due to atmospheric pulsations. Differential line shifts, ΔV _r = 0–8 km/s have been detected on various dates. The position of the molecular spectrum is stationary in time, indicating a constant expansion velocity of the circumstellar shell, V _exp = 15.2 km/s, as derived from the C₂ and NaI lines.     

X Per and V725 Tau: infrared variations on timescales longer than fifteen years

The results of infrared observations of the two Be stars X Per and V725 Tau, which are the optical components of X-ray binary systems, obtained in 1994–2016 are presented. The observations cover Be-star phases as well as shell phases. The data analysis shows that the radiation observed from the binaries at 1.25, 3.5, and 5 μm can be explained as the combined radiation from the optical components and variable sources (shells/disks) that emit as blackbodies (BBs). Emission from a source with the color temperature T _c ~1000?1500 K was detected for X Per at λ ≥ 3.5 μm. The highest IR-brightness variation amplitudes for X Per were 0.9?1.2 ^m (JHK magnitudes) and ~1.45 ^m (LM magnitudes); for V725 Tau, they were 1.1?1.4 ^m and ~1.7 ^m (L magnitudes). The parameters of the optical components and interstellar extinction during the Be phases were estimated: the color excesswasE(B?V) = 0.65±0.08 ^m and 0.77 ± 0.03 ^m for X Per and V725 Tau, respectively. Light from the variable sources (disks/shells) was distinguished and their color temperatures, radii, and luminosities estimated for different observation epochs in a BB model. The variations of the binaries’ IR brightness and colors are shown to be due to changing parameters of the variable sources. The mean color temperature of the cool source (disk/shell) and the mean radius and mean luminosity of X Per are 9500± 2630 K, (35 ± 10) R_⊙, and (9100± 540) L_⊙. For V725 Tau, these parameters are 6200 ± 940 K, (27 ± 6) R_⊙, and (980 ± 420) L_⊙. The 1.25–5 μm radiation from X Per at different epochs can be represented as a sum of contributions from at least three sources: the optical component and two objects emitting as BBs. To reproduce the 1.25–3.5 μm radiation from V725 Tau, two components are sufficient: the optical component and a single variable BB object. For both binary systems, orbital variations of the IR brightness can be noted near the Be-star phase. The amplitudes of the J-band variations of X Per and V725 Tau are about 0.3 ^m and 0.1 ^m , respectively.     

海洋沉积物中的钒、钼、铊、镓及其环境指示意义

研究探讨沉积物中钒、钼、铊和镓的生物地球化学行为对揭示海洋环境演变机制有重要的科学意义,基于此考虑,本文系统分析总结了近年来海洋沉积物中V、Mo、Tl和Ga的地球化学特征以及与环境关系的研究进展,以期对深入开展环境敏感微量元素的海洋生物地球化学有所裨益。结果表明,由于受人为输入的影响,近海沉积物中V、Mo、Tl和Ga含量高于远海,河口高于近海;在表层沉积物中,细颗粒沉积物中V、Mo、Tl和Ga含量高于粗颗粒中的,且其含量与物源、有机质含量等沉积环境因素密切相关;在垂直分布上,随沉积物深度的增加,V、Mo、Tl和Ga含量趋于降低,表明近几十年来,随人为影响的加剧,海洋作为地球上物质的汇获得了比以前更多的V、Mo、Tl和Ga。由此可见,在水平方向上,海洋沉积物中V、Mo、Tl和Ga的丰度可表明输入物源的特性,而在柱状样中的垂直分布,则能够表征历史年代上V、Mo、Tl和Ga沉积量的差异。由于沉积物中V、Mo、Tl和Ga的性质比较稳定,它们在一定程度上可以揭示和表征海洋环境演变的讯息,追溯海洋环境演变的历史以及预测将来的发展趋向。