2017
DOI: 10.1007/s00410-017-1343-3
|View full text |Cite
|
Sign up to set email alerts
|

Heterogeneously entrapped, vapor-rich melt inclusions record pre-eruptive magmatic volatile contents

Abstract: 22Silicate melt inclusions (MI) commonly provide the best record of pre-eruptive H2O and CO2 23 contents of subvolcanic melts, but the concentrations of CO2 and H2O in the melt (glass) phase 24 within MI can be modified by partitioning into a vapor bubble after trapping. Melt inclusions 25 may also enclose vapor bubbles together with the melt (i.e., heterogeneous entrapment), affecting 26 the bulk volatile composition of the MI, and its post-entrapment evolution. Here, we use 27 numerical modeling to examine t… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

2
21
0

Year Published

2017
2017
2025
2025

Publication Types

Select...
6
2

Relationship

0
8

Authors

Journals

citations
Cited by 31 publications
(23 citation statements)
references
References 42 publications
2
21
0
Order By: Relevance
“…The elemental carbon, which is likely present as a thin film coating the inner spherical surface of the bubbles, replaces CO 2 in some samples, probably due to a change in the oxidation state within MIs, for instance related to a diffusive loss of oxygen from the bubbles to the melt, when the latter crystallized oxides during cooling. The large variability in volume and number of bubbles observed in coexisting MIs (ranging from 1 to 25 bubbles per MI, approximately occupying from <0.1 to >0.5 of the MI volume, as optically estimated in thin and thick sections) reveals heterogeneous entrapment of MIs 27,36 . Therefore, the bubbles within MIs are interpreted as gas exsolution bubbles, formed during exsolution of a CO 2 -rich fluid phase likely from the silicate melt prior to, or during, their entrapment.…”
Section: Resultsmentioning
confidence: 96%
“…The elemental carbon, which is likely present as a thin film coating the inner spherical surface of the bubbles, replaces CO 2 in some samples, probably due to a change in the oxidation state within MIs, for instance related to a diffusive loss of oxygen from the bubbles to the melt, when the latter crystallized oxides during cooling. The large variability in volume and number of bubbles observed in coexisting MIs (ranging from 1 to 25 bubbles per MI, approximately occupying from <0.1 to >0.5 of the MI volume, as optically estimated in thin and thick sections) reveals heterogeneous entrapment of MIs 27,36 . Therefore, the bubbles within MIs are interpreted as gas exsolution bubbles, formed during exsolution of a CO 2 -rich fluid phase likely from the silicate melt prior to, or during, their entrapment.…”
Section: Resultsmentioning
confidence: 96%
“…One additional factor that can affect the size of MI bubbles is H + diffusion out of the MI during pre-eruptive (subsurface) cooling. This process results in a lower partial molar volume of the MI, which can lead to contraction of the MI and formation of a bubble 31 . This process cannot be solely responsible for the differences in bubble sizes between Group I and Group II MIs given the similar H 2 O contents of all MIs (Fig.…”
Section: Resultsmentioning
confidence: 99%
“…We can estimate the original dissolved CO 2 content at entrapment for MIs with a co-entrapped exsolved phase by approximating the proportion of dissolved MI CO 2 that sequesters into Group II bubbles during post-entrapment processes. According to models 31 , co-entrapped bubbles suppress exsolution of CO 2 from the melt because they counter some of the pressure loss due to shrinkage of the MI. The degree of suppression of CO 2 exsolution not only depends very strongly on the initial pressure but also on the initial bubble volume fraction and magma composition 31 .…”
Section: Resultsmentioning
confidence: 99%
“…Melt inclusions with vapor bubbles that make up large proportions of the inclusion space (i.e., vapor bubbles that make up >~8–10 vol%), as some in the phenocrysts of our samples (Figures c and b and Table S3), may record the entrapment of two‐phase liquids (silicate melt and an exsolved vapor phase), but they may also record decrepitation or leakage (cf. Bodnar & Student, ; Moore et al, ; Steele‐MacInnis et al, ). The presence of high‐density CO 2 (~0.39–0.75 g/cm 3 ) in some of the high‐volume vapor bubbles (Figure b and Table S3) suggests that a two‐phase liquid was indeed locally trapped (cf.…”
Section: Discussionmentioning
confidence: 99%
“…The presence of high-density CO 2 (~0.39-0.75 g/cm 3 ) in some of the high-volume vapor bubbles (Figure 6b and Table S3) suggests that a two-phase liquid was indeed locally trapped (cf. Steele-MacInnis et al, 2017), and thus that the Menluhe, Xunke, and Wuchagou systems were volatile saturated during phenocryst crystallization. Bubbles in melt inclusions that occupy only~1-6 vol% and on average~3 vol% of the melt inclusion space, in contrast, are interpreted to have formed by postentrapment cooling (cf.…”
Section: Co 2and H 2 O-poor Magmasmentioning
confidence: 99%