Influence of magma ascent rate on carbon dioxide degassing at oceanic ridges: Message in a bubble

Research areas:

• Intérieurs planétaires (2011 - 2016)

Year:

2012

Authors:

• D. Chavrit
• Éric Humler
• Yann Morizet
• D. Laporte

Journal:

EARTH AND PLANETARY SCIENCE LETTERS

Volume:

357

Pages:

376-385

Month:

DEC 1

ISSN:

0012-821X

BibTex:

@article{WOS:000312621600037, author = "D. Chavrit and {\'E}ric Humler and Yann Morizet and D. Laporte", abstract = "In order to quantify the magma ascent rate beneath oceanic ridges, we propose a new method based on vesicle size distribution (VSD) and volatiles measurements (CO2 and H2O) on 65 fresh glasses from the global Mid-Ocean Ridge system. Comparisons of VSD between the main oceanic basins reveal that Mid-Ocean-Ridge-Basalts (MORB) from the Pacific Ocean have significantly higher bubble densities (148(-124)(+739): bubbles/cm(2)) and initial population densities In(n(0))=19.6 +/- 2.8 cm(-4) but lower vesicularities (similar to 0.1%). We determine the residence time of bubbles in the magma using the linear relationship between the logarithm of the density population and the vesicle diameters. Assuming a constant bubble growth rate (G=1.5 x 10(-7) cm/s), we suggest that the transit times of the magmas through the oceanic crust are shorter beneath Pacific ridges (similar to 2 h) than elsewhere (similar to 15 h). In addition, the CO2 and H2O contents of the studied glasses allow the carbon saturation pressure to be calculated. Pacific MORB display a significantly lower carbon dioxide saturation pressure (P-sat = 843(-221)(+300) bars) than Atlantic and Indian MORB (P-sat = 1898(-827)(+1466) bars) but identical pressures of eruption (P-e similar to 310 bars). Consequently, the distance traveled by bubbles from the vesiculation depth to the seafloor is shorter for the Pacific (similar to 1.9 km) than for the Atlantic and Indian oceans (similar to 5.2 km): the longer the transit time, the longer the distance traveled. A closer inspection of the data revealed that the decompression rate (dP/dt) varied from 5.0 X 10(2) to 2.3 X 10(4) Pa/s and correlated positively with the measured bubble densities (nb/m(3)) as expected from experimental data and numerical modeling. At the global scale, most of the Pacific samples are characterized by high ascent rates (0.25(-0.13)(+0.26) m/s) relative to those from the Atlantic (0.11(-0.06)(+0.15) m/s) and the Indian samples (0.09(-0.03)(+0.05) m/s). However, at the local scale some samples from the Mid-Atlantic Ridge at 37 degrees N (where the reflections of seismic waves from crustal magma chamber have been observed) are not distinguishable from the Pacific data set having high ascent rates and large bubble densities. We suggest that the method presented in this study could be used to identify spots along the Mid-Oceanic-Ridge system where magma chambers are possibly present. (C) 2012 Elsevier B.V. All rights reserved.", doi = "10.1016/j.epsl.2012.09.042", extra = "PICL", issn = "0012-821X", journal = "EARTH AND PLANETARY SCIENCE LETTERS", month = "DEC 1", pages = "376-385", title = "{I}nfluence of magma ascent rate on carbon dioxide degassing at oceanic ridges: {M}essage in a bubble", volume = "357", year = "2012", }

Abstract:

In order to quantify the magma ascent rate beneath oceanic ridges, we propose a new method based on vesicle size distribution (VSD) and volatiles measurements (CO2 and H2O) on 65 fresh glasses from the global Mid-Ocean Ridge system. Comparisons of VSD between the main oceanic basins reveal that Mid-Ocean-Ridge-Basalts (MORB) from the Pacific Ocean have significantly higher bubble densities (148(-124)(+739): bubbles/cm(2)) and initial population densities In(n(0))=19.6 +/- 2.8 cm(-4) but lower vesicularities (similar to 0.1%). We determine the residence time of bubbles in the magma using the linear relationship between the logarithm of the density population and the vesicle diameters. Assuming a constant bubble growth rate (G=1.5 x 10(-7) cm/s), we suggest that the transit times of the magmas through the oceanic crust are shorter beneath Pacific ridges (similar to 2 h) than elsewhere (similar to 15 h). In addition, the CO2 and H2O contents of the studied glasses allow the carbon saturation pressure to be calculated. Pacific MORB display a significantly lower carbon dioxide saturation pressure (P-sat = 843(-221)(+300) bars) than Atlantic and Indian MORB (P-sat = 1898(-827)(+1466) bars) but identical pressures of eruption (P-e similar to 310 bars). Consequently, the distance traveled by bubbles from the vesiculation depth to the seafloor is shorter for the Pacific (similar to 1.9 km) than for the Atlantic and Indian oceans (similar to 5.2 km): the longer the transit time, the longer the distance traveled. A closer inspection of the data revealed that the decompression rate (dP/dt) varied from 5.0 X 10(2) to 2.3 X 10(4) Pa/s and correlated positively with the measured bubble densities (nb/m(3)) as expected from experimental data and numerical modeling. At the global scale, most of the Pacific samples are characterized by high ascent rates (0.25(-0.13)(+0.26) m/s) relative to those from the Atlantic (0.11(-0.06)(+0.15) m/s) and the Indian samples (0.09(-0.03)(+0.05) m/s). However, at the local scale some samples from the Mid-Atlantic Ridge at 37 degrees N (where the reflections of seismic waves from crustal magma chamber have been observed) are not distinguishable from the Pacific data set having high ascent rates and large bubble densities. We suggest that the method presented in this study could be used to identify spots along the Mid-Oceanic-Ridge system where magma chambers are possibly present. (C) 2012 Elsevier B.V. All rights reserved.