scholarly journals Light elements, volatiles, and stable isotopes in basaltic melt inclusions from Grenada, Lesser Antilles: Inferences for magma genesis

2010 ◽  
Vol 11 (9) ◽  
Author(s):  
A.-S. Bouvier ◽  
N. Métrich ◽  
E. Deloule
1959 ◽  
pp. 113-119
Author(s):  
N. M. Zhavoronkov ◽  
O. V. Uvarov ◽  
S. I. Babkov

2009 ◽  
Vol 33 (-1) ◽  
pp. 33-36 ◽  
Author(s):  
Algirdas Gaigalas ◽  
Stanislaw Halas

Stable Isotopes (H, C, S) and the Origin of Baltic Amber New results of isotope analysis of light elements (H, C and S) of a dozen Baltic amber samples are described and discussed. Carbon isotope composition was nearly constant (ca. -23‰), whereas sulphur and hydrogen varied in their isotope compositions from +4 to -28‰ and from -171 to -213‰, respectively. The formation and subsequent evolution of this material since its origin in Paleogene time until present is outlined.


2021 ◽  
Author(s):  
◽  
Katharine Emma Saunders

<p>The petrogenesis of silicic arc magmas is controversial with end-member models of fractional crystallisation and crustal anatexis having been invoked. A prime example of this is the archetypical continental Taupo Volcanic Zone and the adjacent oceanic Kermadec Arc. Insights into the genesis and timescales of magmatic processes of four continental rhyolitic magmas (Whakamaru, Oruanui, Taupo and Rotorua eruptives) and an oceanic (Healy seamount) rhyodacitic magma are documented through micro-analytical chemical studies of melt inclusions and crystal zonation of plagioclase and quartz. Electron probe microanalysis, laser ablation inductively coupled plasma mass spectrometry and Fourier transform infrared spectroscopy have been used to measure major, trace and volatile element concentrations, respectively, of melt inclusions and crystals. Melt inclusions are high silica (e.g. 74 - 79 wt%) irrespective of arc setting and display a wide range of trace element compositions (e.g. Sr = 17 - 180 ppm). Taupo Volcanic Zone melt inclusions exhibit higher K2O and Ce/Yb relative to Healy melt inclusions reflecting the assimilation of continental lithosphere. Quantitative trace element modelling of melt inclusion compositions: (a) demonstrates that magma genesis occurred through 62 - 76% fractional crystallisation at Healy whereas assimilation of continental lithosphere (greywacke) in addition to 60 - 80% fractional crystallisation is required for the Taupo Volcanic Zone magmas; and (b) suggests the presence of crystal mush bodies beneath silicic magma chambers in both continental and oceanic arc environments. Water concentrations of melt inclusions ranged between 1.4 - 5.1 wt% for the Whakamaru, Taupo and Healy samples. However, the inconsistency in the measured molecular water to hydroxyl concentrations of melt inclusions relative to those determined experimentally for groundmass rhyolitic glasses provide evidence for the degassing of inclusions prior to quenching, by diffusion of hydroxyl groups through the crystal host. Thus, partial pressures of water estimated from the inclusions and inferred depths of the crystallising magma bodies are underestimated. Chemical profiles of mineral zonation, however, indicate a more complex origin of silicic melts than simple fractionation and assimilation. For example, trace element modelling of Whakamaru plagioclase suggests that the three distinct textural plagioclase populations present in Whakamaru samples crystallised from four physiochemically discrete silicic melts. This modelling indicates a strong petrogenetic link between andesitic and silicic magmas from the chemical variation of selected Whakamaru plagioclase crystals possessing high anorthite (45-60 mol %) cores and low anorthite (~ 30 mol %) rim compositions and the interaction of greywacke partial melts. Furthermore, Sr diffusion modelling of core-rim interfaces of the same plagioclase crystals indicate the amalgamation of the magma chamber occurred continuously over the 15,000 years preceding the climactic eruption. Conversely, the major element zonation of Taupo plagioclases implies magma genesis occurred solely through assimilation and fractional crystallisation without the incorporation of evolved crystal mush magmas, indicating a spectrum of magmatic processes are occurring beneath the Taupo Volcanic Zone with each eruption providing only a snapshot of the petrogenesis of the Taupo Volcanic Zone.</p>


2006 ◽  
Vol 70 (6) ◽  
pp. 669-687 ◽  
Author(s):  
Khin Zaw ◽  
F. L. Sutherland ◽  
F. Dellapasqua ◽  
C. G. Ryan ◽  
Tzen-Fu Yui ◽  
...  

AbstractCorundum xenocrysts from alkaline basalt fields differ in characteristics and hence lithospheric origins. Trace element, fluid/melt inclusion and oxygen isotope studies on two eastern Australian corundum deposits are compared to consider their origins. Sapphires from Weldborough, NE Tasmania, are magmatic (high-Ga, av. 200 ppm) and dominated by Fe (av. 3300 ppm) and variable Ti (av. 400 ppm) as chromophores. They contain Cl, Fe, Ga, Ti and CO2-rich fluid inclusions and give δ18O values (5.1–6.2‰) of mantle range. Geochronology on companion zircons suggests several sources (from 290 Ma to 47 Ma) were disrupted by basaltic melts (47 ± 0.6 Ma). Gem corundums from Barrington, New South Wales, also include magmatic sapphires (Ga av. 170 ppm; δ18O (4.6–5.8‰), but with more Fe (av. 9000 ppm) and less Ti (av. 300 ppm) as chromophores. Zircon dating suggests that gem formation preceded and was overlapped by Cenozoic basaltic melt generation (59–4 Ma). In contrast, a metamorphic sapphire-ruby suite (low-Ga, av. 30 ppm) here incorporates greater Cr into the chromophores (up to 2250 ppm). Fluid inclusions are CO2-poor, but melt inclusions suggest some alkaline melt interaction. The δ18O values (5.1–6.2‰) overlap magmatic sapphire values. Interactions at contact zones (T = 780–940°C) between earlier Permian ultramafic bodies and later alkaline fluid activity may explain the formation of rubies.


2010 ◽  
Vol 26 (8) ◽  
pp. 873-878 ◽  
Author(s):  
Takashi KORENAGA ◽  
Masaaki MUSASHI ◽  
Rumiko NAKASHITA ◽  
Yaeko SUZUKI

1975 ◽  
Vol 189 (1095) ◽  
pp. 183-211 ◽  

Isotopic distribution is a function of physical and biological processes. In general, equilibrium-controlled reactions occur at high temperatures among solid phases, whereas low-temperature reactions, especially those mediated by organisms, are kinetically controlled. The solar and stellar abundance of isotopes is poorly known. Knowledge of extra-terrestrial distributions of the isotopes of light elements presently comes from lunar and meteorite measurements. On Earth, the elements associated with biological synthesis which have been studied most intensively, are hydrogen, carbon, nitrogen, oxygen and sulphur. In general, reduced products of metabolism are enriched in light isotopes. Thus, 1 H and 12 C are enriched in hydrogen gas and methane, when produced by fermentation or CO 2 reduction. Nitrogen gas is enriched in 14 N when produced by denitrification, and H 2 S is highly enriched in 32 S when it results from sulphate reduction. A pattern of biological enrichment factors has been recognized on Earth, but until now, not in lunar or meteorite samples.


2006 ◽  
Vol 70 (18) ◽  
pp. A284
Author(s):  
M.G. Jackson ◽  
S.R. Hart ◽  
L. Ball

Author(s):  
A. Meliashchenia ◽  
T. Senchenko ◽  
T. Smaliak ◽  
T. Savelieva ◽  
M. Korkina

Samples of milk, water, and feed for farm animals were studied to determine the ratio of stable isotopes of the light elements carbon δ13C, oxygen δ18O, nitrogen δ15N. Samples were selected in different geographical and climatic zones of the Republic of Belarus. It was found that the isotopic composition of milk varies in different regions depending on the diet of animals and the season.


Author(s):  
Paul J. Wallace ◽  
Terry Plank ◽  
Robert J. Bodnar ◽  
Glenn A. Gaetani ◽  
Thomas Shea

Inclusions of basaltic melt trapped inside of olivine phenocrysts during igneous crystallization provide a rich, crystal-scale record of magmatic processes ranging from mantle melting to ascent, eruption, and quenching of magma during volcanic eruptions. Melt inclusions are particularly valuable for retaining information on volatiles such as H2O and CO2 that are normally lost by vesiculation and degassing as magma ascends and erupts. However, the record preserved in melt inclusions can be variably obscured by postentrapment processes, and thus melt inclusion research requires careful evaluation of the effects of such processes. Here we review processes by which melt inclusions are trapped and modified after trapping, describe new opportunities for studying the rates of magmatic and volcanic processes over a range of timescales using the kinetics of post-trapping processes, and describe recent developments in the use of volatile contents of melt inclusions to improve our understanding of how volcanoes work. ▪ Inclusions of silicate melt (magma) trapped inside of crystals formed by magma crystallization provide a rich, detailed record of what happens beneath volcanoes. ▪ These inclusions record information ranging from how magma forms deep inside Earth to its final hours as it ascends to the surface and erupts. ▪ The melt inclusion record, however, is complex and hazy because of many processes that modify the inclusions after they become trapped in crystals. ▪ Melt inclusions provide a primary archive of dissolved gases in magma, which are the key ingredients that make volcanoes erupt explosively. Expected final online publication date for the Annual Review of Earth and Planetary Sciences, Volume 49 is May 2021. Please see http://www.annualreviews.org/page/journal/pubdates for revised estimates.


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