Liquidus temperatures and phase compositions in the system Qz-Ab-Or at 5 kbar and very low water activities

Liquidus phase relations have been experimentally determined in the systems Qz-Ab-Or-(H₂O), Qz-Ab-(H₂O) and Qz-Or-(H₂O) at H₂O-undersaturated conditions (a _H2O = 0.07) and P = 5 kbar. Starting materials were homogeneous synthetic glasses containing 1 wt% H₂O. The liquidus temperatures were bracketed by crystallization and dissolution experiments. The results of kinetic studies showed that crushed glasses are the best starting materials to overcome undercooling and to minimize the temperature difference between the lowest temperature of complete dissolution (melting) and the highest temperature at which crystallization can be observed. At P = 5 kbar and a _H2O = 0.07, the Qz-Ab eutectic composition is Qz₃₂Ab₆₈ at 1095 °C (±10 °C) and the Qz-Or eutectic is Qz₃₈Or₆₂ at 1030 °C (±10 °C). The minimum temperature of the ternary system Qz-Ab-Or is 990 °C (±10 °C) and the minimum composition is Qz₃₂Ab₃₅‐ Or₃₃. The Qz content of the minimum composition in the system Qz-Ab-Or-H₂O remains constant with changing a _H2O. The normative Or content, however, increases by approximately 10 wt% with decreasing a _H2O from 1 to 0.07. Such an increase has already been observed in the system Qz-Ab-Or-H₂O-CO₂ at high a _H2O and it is concluded that the use of CO₂ to reduce water activities does not influence the composition of the minima in quartz-feldspar systems. The determined liquidus temperature in melts with 1 wt% H₂O is very similar to that obtained in previous nominally “dry” experiments. This discrepancy is interpreted to be due to problems in obtaining absolutely dry conditions. Thus, the hitherto published solidus and liquidus temperatures for “dry” conditions are probably underestimated. Received: 27 March 1997 / Accepted: 1 October 1997     

Formation and ascent of granitic magmas

New results obtained by the investigation of liquidus and solidus phase relationships in the haplogranite system Qz-Ab-Or are used to discuss the evolution of magmas during their ascent in the crust. It is assumed that the magmas are formed at 720°C, 820°C, 920°C and at a depth corresponding to a pressure of 8 kbar. The starting composition of the magma is taken as 50% melt plus 50% quartz and feldspars. In case of a closed system (no heat exchange and no transfer of elements) the melt fraction of magmas, the water activity and the viscosity increase with decreasing pressure. The temperature slightly decreases. At 700°C the viscosity is approximatively 2 orders of magnitude lower than at 900°C. This is related to the higher amount of water in the (H₂O-undersaturated) melt at low T. It is also shown that dehydration melting is only realistic at high T (900°C). At lower temperatures water has to be added from outside to obtain an intrusive magma with approximatively 50% melt.

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Zusammenfassung Neue Ergebnisse, erzielt durch Untersuchungen von Liquidus und Solidus Phasenbeziehungen des Granitsystems Qz-Ab-Or, werden benutzt, um die Entwicklung eines granitoiden Magmas während seines Aufstiegs zu diskutieren. Es wird vorausgesetzt, daß die Magmen bei Temperaturen von 720°C, 820°C und 920°C gebildet werden, sowie in einer Tiefe die einem Druck von 8 kbar entspricht. Die anfängliche Zusammensetzung des Magmas wird mit einem Verhältnis von 50% Schmelze sowie 50% Quarz und Feldspäten angenommen. Im Falle eines geschlossenen Systems (kein Austausch von Wärme und Elementen) steigt die Teilschmelzbildung von Magmen, die Aktivität des Wassers und die Viskosität bei abnehmenden Druck; hierbei sinkt die Temperatur leicht. Bei 700°C ist die Viskosität um ca. 2 Größenordnungen geringer als bei 900°C. Dies wird bedingt durch den höheren Gehalt an Wasser in der (H₂O-untersättigten) Schmelze bei tieferen Temperaturen. Es wird außerdem gezeigt, daß Magmenbildung durch Dehydratation nur bei hohen Temperaturen realistisch ist (900°C). Bei tieferen Temperaturen muß Wasser von außen zugeführt werden um ein intrusives Magma zu erhalten, das ungefähr 50% Schmelze besitzt.

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Résumé L'évolution des magmas granitiques au cours de leur ascension dans la croûte est discutée à la lumière de données nouvelles relatives aux relations entre phases liquides et solides dans le système Q-Ab-Or. On suppose que les magmas se forment à des températures de 720°C, 820°C, 920°C et à une profondeur correspondant à une pression de 8 Kb. On admet pour leur composition initiale un mélange de 50% de liquide et 50% de quartz + feldspaths. Dans le cas d'un système fermé (pas d'échange de chaleur ni de matière), la fraction liquide du magma, l'activité de l'eau et la viscosité augmentent quand la pression diminue; en même temps, la température décroît légèrement. A 700°C, la viscosité est d'environ 2 ordres de grandeur plus basse qu'à 900°C. Cette propriété est en relation avec la teneur en eau plus élevée dans le liquide (sous-saturé en eau) à basse température. On peut également montrer qu'une fusion déshydratante n'est vraisemblable qu'à haute température (900°C). Aux températures plus basses, de l'eau doit être apportée de l'extérieur pour l'obtention d'un magma à 50% de liquide.

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Verbreitung und Ausbildung der Siegener Schichten in der Osteifel

Ohne ZusammenfassungVortrag, gehalten auf der Hauptversammlung der Geologischen Vereinigung zu Frankfurt a. M., Januar 1933.     

V. Bücher- und Zeitschriftenschau

Ohne Zusammenfassung     

Die Graubündner Erdbeben und Wetterstürze im August 1927

Ohne Zusammenfassung     

Das Vorland der Alpen und die Vorgeschichte der Alpenfaltung

Ohne Zusammenfassung     

A laboratory study of Equotip surface hardness measurements on a range of sandstones: What influences the values and what do they mean?

The Equotip rebound tester is a simple, non-destructive technique to measure the surface hardness of materials. Having a low impact energy gives the Equotip advantages over the commonly used Schmidt Hammer on weathered rock and stone. In this study we have investigated the influence of different parameters (sample size, moisture content and surface roughness) on the surface hardness values obtained from freshly cut blocks of four types of sandstone. In a series of laboratory experiments both Single Impacts (SIM) and Repeat Impacts (RIM) methods have been used with C and D probes (which have different impact energies). Our results show that whilst sample size is of great importance we find that smaller samples can be reliably evaluated than previously reported. Moisture contents are also found to exert a more important influence on both SIM and RIM results than previously thought, with up to 26% lower hardness values recorded on saturated vs dry sandstone. Conversely, we find that surface roughness (over Sz values of 100 to 800 microns) does not have a significant impact on SIM measurements collected using the D probe. Both SIM and RIM data are found to be good proxies for compressive strength and open porosity, with SIM data collected with the C probe showing the best fits. Data collected using 3D microscopy helps visualize and quantify the small impact marks created by the Equotip and confirms that these are much reduced when using the C vs D probe. The results highlight the benefits of the Equotip to studies of the nature and deterioration of sandstone, the need for careful evaluation of any confounding factors which might influence the values obtained, and illustrate the different advantages of C and D probes. © 2019 John Wiley & Sons, Ltd.     

Influence of soil properties on active layer thermal propagation along the western Antarctic Peninsula

The rate of energy transfer through soils is an important factor governing the active layer (seasonal thaw layer) in polar regions. Energy is transferred through conductive and convective means, which are primarily influenced by the bulk density and water content of soils. With global temperatures changing, it becomes important to understand how soil properties influence heat transfer and active layer depths in climatically sensitive regions, such as the Antarctic Peninsula. In this study we analyzed conductive energy transfer through several soil types on Amsler Island and Cierva Point in the central region of the western Antarctic Peninsula. Active layer temperatures on Amsler Island were monitored every three hours using iButton thermistors installed at regular depth intervals down to 2 m. Soil textures were loamy to sandy with water contents between 5 and 27%. Freezing and thawing transmission rates for all soils ranged from 1.4 to 6.9 cm/day. Thermal transmission rates were fastest in sandy soils with low water contents, indicating that the large, interconnected pores of the sandy soils facilitated the quick movement of heat with water flow through the soil profile. Snow accumulation differences also played a significant role on winter thermal propagation by providing a thermal barrier between the ground surface and atmosphere. Although there was a wide range in thermal transmission among the soils, active layer depths had little variation (7.8–9.7 m). This consistency derives from the greater dependence of very thick active layers on long‐term climatic conditions rather than on soil properties. The presence of thick moss significantly slowed thermal transmission and decreased active layer thicknesses. These effects primarily are due to the high heat capacity of water and air retained within the moss, slowing thermal transmission rates, acting as a thermal buffer between atmospheric conditions and the underlying soils. Copyright © 2016 John Wiley & Sons, Ltd.