Quantitative vesicle analyses and total CO2 reconstruction in mid-ocean ridge basalts
Introduction
Mid-ocean ridge basalts (MORB) frequently experience incomplete degassing due to the hydrostatic pressure at the seafloor. As a result, MORB volatile concentrations can provide valuable insight into volatile abundances in Earth's upper mantle (e.g., Cartigny et al., 2008; Jones et al., 2019; Michael and Graham, 2015), which influence mantle melting, melt migration, and geophysical properties of the Earth's interior (e.g., Dasgupta and Hirschmann, 2010; Hirth and Kohlstedt, 1996). MORB CO2 concentrations and vesicle textures have also been used to constrain mid-ocean ridge CO2 flux (e.g., Chavrit et al., 2014), magma storage conditions within the oceanic crust (e.g., Aubaud et al., 2004; Dixon et al., 1988; le Roux et al., 2006; Sarda and Graham, 1990) and magma ascent and effusion rates during mid-ocean ridge eruptions (Chavrit et al., 2012; Gardner et al., 2016; Jones et al., 2018; Soule et al., 2012). Many of these studies estimate 3D vesicularities and reconstruct total CO2 concentrations using 2D measurements (e.g., Aubaud et al., 2004; Chavrit et al., 2014; Hekinian et al., 2000; Javoy and Pineau, 1991; Jones et al., 2018; Pineau et al., 2004; Soule et al., 2012). However, the methods for reconstructing 3D vesicle textures and total CO2 concentrations in MORB have not yet been rigorously tested. Aubry et al. (2013) highlight the sensitivity of CO2 reconstructions to assumptions regarding the behavior of vesicles during quenching, suggesting that improper assumptions may explain systematic differences between calculated and simulated CO2 contents in a suite of MORB samples. Several studies compare 2D and 3D vesicularities and vesicle size distributions in subaerial samples (Baker et al., 2011; Giachetti et al., 2011; Gurioli et al., 2008; Hughes et al., 2017); however, MORB have different vesicle characteristics than most subaerial samples, including low vesicularities (i.e., gas volume fractions), low vesicle number densities (i.e., number of vesicles per unit volume), and small vesicle sizes, which motivates a robust evaluation of these methods specific to MORB.
This study examines theoretical and empirical methods for quantifying vesicle populations in a suite of MORB samples and offers new insights into the validity of those methods and best practices for evaluating vesicularity, vesicle size distributions, and CO2 concentrations in this subgroup of volcanic rocks. We use comparative 2D and 3D measurements of MORB samples along with synthetic data to provide a consistent, comprehensive evaluation of stereological corrections in MORB. We further suggest an improved method for quantifying exsolved CO2 concentrations based on vesicularity through an evaluation of equations of state, theoretical estimates of vesicle volume change during cooling, and estimates of CO2(g) density in MORB samples based on Raman spectroscopy.
Section snippets
Stereological corrections
Stereology allows the determination of volumetric vesicle number densities and size distributions from cross-sectional measurements. The mathematical formulations and limitations of stereology are reviewed in Dehoff and Rhines (1968), Hilliard and Lawson (2003), Russ (1986), Underwood (1970) and Vander Voort (1999). Several papers have focused on the application of stereology to vesicle size distributions (e.g. Cashman and Mangan, 1994; Sahagian and Proussevitch, 1998; Shea et al., 2010) and
Samples
The MORB glasses analyzed for vesicularity and vesicle size distributions were collected from Axial Seamount on the Juan de Fuca Ridge (N = 8; sample descriptions in Jones et al. (2018)) and near 13.75°N on the Mid-Atlantic Ridge (N = 12; sample descriptions in Jones et al. (2019)). The methods for calculating total CO2 concentrations in MORB were evaluated using samples from the 2011 eruption of Axial Seamount on the Juan de Fuca Ridge. The published 2D vesicularity measurements and dissolved
Qualitative visual observations
The following visual observations were made based on the reflected light photomicrographs and reconstructed X-ray μ-CT scans (Fig. 1). The visually estimated crystallinity is <2% for all samples. The crystals are commonly clustered and often touching vesicles. All samples display similar vesicle textures. Small vesicles (<250 μm radius) appear mostly spherical while larger vesicles appear occasionally elongated (Fig. 1c). The smallest vesicles (<20 μm radius) are often clustered near crystals (
Optimal sample size and spatial resolution for MORB vesicularity studies
The inherent trade-off between X-ray μ-CT resolution and sample volume analyzed can impact the measured vesicularity and vesicle number density. Two of the three samples scanned at multiple resolutions demonstrate that analyzing too small of a sample volume, despite the potential for improved resolution, can produce erroneous vesicularities and vesicle size distributions. The limited sample volume likely caused the apparent truncation of the vesicle size distributions and vesicle volume
Conclusions
We demonstrate that 2D analyses combined with stereological techniques accurately reproduce vesicularities and vesicle size distributions in MORB given sufficient sample sizes and replicate measurements. For accurate 2D results, we recommend measuring multiple fragments from each sample and analyzing a total fragment area >100 times the area of the largest measured bubble. We further recommend analyzing at least 200 vesicles for accurate vesicle size distributions using the stereological method
Code availability
Code for reproducing the results from this study will be published at https://github.com/maxrjones/MORB-CO2-vesicles upon acceptance.
Author contributions
MPJ, SS, VLR, and HB contributed vesicularity/VSD data; MPJ and FK contributed Raman spectroscopy data; MPJ and HB contributed synthetic data; MPJ and YL modeled quenching. MPJ led data processing, interpretation, and writing with contributions from all co-authors.
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgments
We are thankful to the captain, crew, vehicle teams, and science participants of the R/V Thompson VISIONS’11 cruise, R/V Western Flyer Northern Expeditions cruises, and R/V Atlantis AT33-03 cruise for collecting the samples used in this study. We thank T. Grove, D. Lizarralde, M. Kurz, T. Perron, M. Manga, and D. Wanless for insightful comments on earlier versions of this work. We thank R. Bodnar, G. Gaetani, H. Lamadrid, A. Pamukcu, and T. Shea for helpful conversations. We thank D. Graham and
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