Effects of superheating magnitude on olivine growth

שמור ב:
מידע ביבליוגרפי
הוצא לאור ב:Contributions to Mineralogy and Petrology vol. 175, no. 2 (Feb 2020)
מחבר ראשי: First, Emily C
מחברים אחרים: Leonhardi, Tanis C, Hammer, Julia E
יצא לאור:
Springer Nature B.V.
נושאים:
גישה מקוונת:Citation/Abstract
Full Text - PDF
תגים: הוספת תג
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MARC

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100 1 |a First, Emily C  |u University of Hawai‘i at Mānoa, Department of Geology and Geophysics, Honolulu, USA (GRID:grid.410445.0) (ISNI:0000 0001 2188 0957); Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, USA (GRID:grid.40263.33) (ISNI:0000 0004 1936 9094) 
245 1 |a Effects of superheating magnitude on olivine growth 
260 |b Springer Nature B.V.  |c Feb 2020 
513 |a Journal Article 
520 3 |a Magmatic superheating is a condition with relevance to natural systems as well as experimental studies of crystallization kinetics. Magmas on Earth and other planetary bodies may become superheated during adiabatic ascent from the mantle or as a consequence of meteorite impact-generated crustal melting. Experimental studies of igneous processes commonly employ superheating in the homogenization of synthetic starting materials. We performed 1-atmosphere dynamic crystallization experiments to study the effects of superliquidus thermal history on the morphologies and compositions of subsequently grown olivine crystals. An ultramafic volcanic rock with abundant olivine was fused above the experimentally determined liquidus temperature (1395 °C), held for 0, 3, or 12 h, cooled at 25 °C h−1, and quenched from 200 °C below the liquidus, all at constant fO2, corresponding to FMQ-2 ± 0.2 log units. An increase in olivine morphologic instability is correlated with superheating magnitude, parameterized as the integrated time the sample is held above the liquidus (“TtL”;  °C h). We infer that a delay in nucleation, which intensifies monotonically with increasing TtL, causes crystal growth to be increasingly rapid. This result indicates that the structural relaxation time scale controlling the formation of crystal nuclei is (a) far longer than the time scale associated with viscous flow and (b) exceeds the liquidus dwell times typically imposed in crystallization experiments. The influence of magmatic superheating on crystal morphology is similar in sense and magnitude to that of subliquidus cooling rate and thus, both factors should be considered when interpreting the thermal history of a volcanic rock containing anhedral olivine. 
653 |a Crystal structure 
653 |a Nucleation 
653 |a Volcanic rocks 
653 |a Olivine 
653 |a Crystallization 
653 |a Lava 
653 |a Meteorite collisions 
653 |a Kinetics 
653 |a Crystal growth 
653 |a Superheating 
653 |a Cooling rate 
653 |a Time 
653 |a Ascent 
653 |a Magma 
653 |a Crystals 
653 |a Viscous flow 
653 |a Relaxation time 
653 |a Earth 
653 |a Dwell time 
653 |a Liquidus 
653 |a Crystal morphology 
653 |a Mineralogy 
653 |a Petrology 
653 |a Environmental 
700 1 |a Leonhardi, Tanis C  |u University of Hawai‘i at Mānoa, Department of Geology and Geophysics, Honolulu, USA (GRID:grid.410445.0) (ISNI:0000 0001 2188 0957); University of California, Berkeley, Department of Earth and Planetary Science, Berkeley, USA (GRID:grid.47840.3f) (ISNI:0000 0001 2181 7878) 
700 1 |a Hammer, Julia E  |u University of Hawai‘i at Mānoa, Department of Geology and Geophysics, Honolulu, USA (GRID:grid.410445.0) (ISNI:0000 0001 2188 0957) 
773 0 |t Contributions to Mineralogy and Petrology  |g vol. 175, no. 2 (Feb 2020) 
786 0 |d ProQuest  |t Science Database 
856 4 1 |3 Citation/Abstract  |u https://www.proquest.com/docview/2343362513/abstract/embedded/75I98GEZK8WCJMPQ?source=fedsrch 
856 4 0 |3 Full Text - PDF  |u https://www.proquest.com/docview/2343362513/fulltextPDF/embedded/75I98GEZK8WCJMPQ?source=fedsrch