Rubidium-Strontium-Altersbestimmungen an Biotit-Muskowit-Granitgneisen (Typus Augen- und Flasergneise) aus dem nördlichen Großvenedigerbereich (Hohe Tauern)

Zusammenfassung An vier Proben aus dem Augen- und Flasergneiskomplex in Großvenedigergebiet (Hohe Tauern) wurden Rb–Sr-Altersbestimmungen durchgeführt. Die Biotit-Alterswerte lagen bei zirka 20 M. J. Sie sind der alpidischen Tauernkristallisation zuzuordnen. Eine Gesamtgesteinsisochrone von drei typischen Augen- und Flasergranitgneisen ergab 246 M. J. und wird als Bildungsalter eines magmatischen Granitkörpers interpretiert. Es muß daher zur Perm-Zeit in den westlichen Hohen Tauern ein ausgedehnter Granitmagmatismus angenommen werden. Auf die Schwierigkeiten, dieses Ereignis in das derzeitige geologische-Entstehungsbild einzuordnen, wurde hingewiesen.

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Rubidium-strontium age determinations on biotite-muscovite-gneisses (Augen-and Flaser-gneisses) from the Northern Grossvenediger region (Tauern, Austrian Alps)

Summary Rb–Sr ages were determined for 4 samples from the Augen- and Flaser-gneiss complex of the Grossvenediger region, Hohe Tauern, Austria. The biotite ages of 20 m. y. may be attributed to the Tauern-crystallization of Alpidic age. A total rock isochrone of 246 m. y. based on 3 typical Augen- and Flaser-granite gneisses is interpreted as the age of a granite body. Thus extensive granite magmatism is assumed to have prevailed in the western part of the Hohe Tauern during the Permian. There are, however, difficulties in correlating this event with the present picture of the geologic evolution in this region.

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On the maintenance of the atmosphere's kinetic energy over the Northern Hemisphere in winter

Summary A quantitative study of the balance requirements of the atmosphere's kinetic energy during normal winter conditions is made for the whole Northern Hemisphere and separately for the tropics (0–30°N) and the extratropics (30–90°N) by using different sources of data. The most important new finding is a demonstration of the existence (on the isobaric surfaces) of meridional eddy flux of potential energy; this flux approximately counterbalances the meridional flux of kinetic energy. One of the conclusions reached is that maintenance of the large-scale eddies in the tropics is mainly due to forcing by extratropical eddies. This forcing occurs at 30°N as a southward eddy flux of potential energy.     

Geophysical investigations on manned spacecrafts

Summary Review has been made of the first results and perspectives of investigations in geophysics and bordering sciences (geology, geography, agrobiology, etc.) by means of manned orbital space laboratories. Relatively detailed discussion is given to the problems of the interpretation of terrain feature pictures from space. Attentively considered are the technique and results of the photometric processing of atmospheric photographs near the horizon with the purpose of studying atmospheric optical non-homogeneities (in particular, aerosol layers). The possible investigations based on the use of data about the outgoing radiation spectra are mentioned. (, , .) . . ( , ) . .     

An empirical NaKCa geothermometer for natural waters

An empirical method of estimating the last temperature of water-rock interaction has been devised. It is based upon molar Na, K and Ca concentrations in natural waters from temperature environments ranging from 4 to 340°C. The data for most geothermal waters cluster near a straight line when plotted as the function $\text{log (}\text{Na}\text{K}\text{) + β log [ √}\text{(Ca)}\text{Na}\text{]}$ vs reciprocal of absolute temperature, where β is either $\text{1}\text{3}$ or $\text{4}\text{3}$ depending upon whether the water equilibrated above or below 100°C. For most waters tested, the method gives better results than the $\text{Na}\text{K}$ methods suggested by other workers. The ratio $\text{Na}\text{K}$ should not be used to estimate temperature if $\text{√ (}\text{M}{}_{\mathrm{Ca}}\text{)}\text{M}{}_{\mathrm{Na}}$ is greater than 1. The $\text{Na}\text{K}$ values of such waters generally yield calculated temperatures much higher than the actual temperature at which water interacted with the rock.A comparison of the composition of boiling hot-spring water with that obtained from a nearby well (170°C) in Yellowstone Park shows that continued water-rock reactions may occur during ascent of water even though that ascent is so rapid that little or no heat is lost to the country rock, i.e. the water cools adiabatically. As a result of such continued reaction, waters which dissolve additional Ca as they ascend from the aquifer to the surface will yield estimated aquifer temperatures that are too low. On the other hand, waters initially having enough Ca to deposit calcium carbonate during ascent may yield estimated aquifer temperatures that are too high if aqueous Na and K are prevented from further reaction with country rock owing to armoring by calcite or silica minerals.The Na-K-Ca geothermometer is of particular interest to those prospecting for geothermal energy. The method also may be of use in interpreting compositions of fluid inclusions.     

Lead orthophosphates—III. Stabilities of fluoropyromorphite and bromopyromorphite at 25°C

The reactions of secondary lead orthophosphate with approximately 10^?1 M sodium fluoride and sodium bromide solutions have been investigated at 25°C. Interpretation of the solubility data resulted in solubility product constants for fluoropyromorphite and bromopyromorphite of 10^?71.6 and 10^?78.1, respectively. According to these constants, the stability sequence for lead pyromorphites is Pb₅(PO₄)₃Cl > Pb₅(PO₄)₃Br > Pb₅(PO₄)₃OH > Pb₅(PO₄)₃F. The derived free energy data have been used to evaluate the respective stabilities of fluoro-pyromorphite and bromopyromorphite within the systems PbF₂-PbO-P₂O₅-H₂O and PbBr₂-PbO-P₂O₅-H₂O and to predict the equilibrium behavior of the Pb₅(PO₄)₃F-Pb₅(PO₄)₃OH solid solution under aqueous conditions.     

Luna 20: mineralogy and petrology of fragments less than 125 μm size

Two milligrams of less than 125 μm size particles from the Luna 20 soil sample (22001,17) have been examined. The results of the mineral identification and analysis verify earlier assumptions that the nature of the lunar highlands is predominantly anorthositic in composition. The presence of highly magnesian clinopyroxene, orthopyroxene and olivine suggests crystallization of Highland rocks in an ultrabasic environment. No fragments were observed that could be unequivocally assigned to mare basalt types.