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  5. Geochemistry and volatile content of magmas feeding explosive eruptions at Telica volcano (Nicaragua)
 
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Geochemistry and volatile content of magmas feeding explosive eruptions at Telica volcano (Nicaragua)

Author(s)
Robidoux, Philippe  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia  
Rotolo, Silvio Giuseppe  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia  
Aiuppa, A.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia  
Lanzo, Giovanni  
Università di Palermo  
Hauri, Erik  
Carnegie Institution, Dept. Terrestrail magnetism  
Language
English
Obiettivo Specifico
1V. Storia eruttiva
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Journal of Volcanology and Geothermal Research  
Issue/vol(year)
/341 (2017)
ISSN
0377-0273
Publisher
Elsevier
Pages (printed)
131-148
Date Issued
July 15, 2017
DOI
10.1016/j.jvolgeores.2017.05.007
URI
https://www.earth-prints.org/handle/2122/10601
Subjects
04.08. Volcanology  
Subjects

Telica, Nicaragua

Abstract
Telica volcano, in north-west Nicaragua, is a young stratovolcano of intermediate magma composition producing
frequent Vulcanian to phreatic explosive eruptions. The Telica stratigraphic record also includes examples of
(pre)historic sub-Plinian activity. To refine our knowledge of this very active volcano, weanalyzedmajor element
composition and volatile content of melt inclusions fromsomestratigraphically significant Telica tephra deposits.
These include: (1) the Scoria Telica Superior (STS) deposit (2000 to 200 years Before Present; Volcanic Explosive
Index, VEI, of 2–3) and (2) pyroclasts from the post-1970s eruptive cycle (1982; 2011). Based on measurements
with nanoscale secondary ion mass spectrometry, olivine-hosted (forsterite [Fo] N 80) glass inclusions fall into 2
distinct clusters: a group of H2O-rich (1.8–5.2 wt%) inclusions, similar to those of nearby Cerro Negro volcano,
and a second group of CO2-rich (360–1700 μg/g CO2) inclusions (Nejapa, Granada). Model calculations show
that CO2 dominates the equilibrium magmatic vapor phase in the majority of the primitive inclusions (XCO2 N
0.62–0.95). CO2, sulfur (generally b2000 μg/g) and H2O are lost to the vapor phase during deep decompression
(P N 400 MPa) and early crystallization of magmas. Chlorine exhibits a wide concentration range (400–2300
μg/g) in primitive olivine-entrapped melts (likely suggesting variable source heterogeneity) and is typically
enriched in the most differentiated melts (1000–3000 μg/g). Primitive, volatile-rich olivine-hosted melt inclusions
(entrapment pressures, 5–15 km depth) are exclusively found in the largest-scale Telica eruptions (exemplified
by STS in our study). These eruptions are thus tentatively explained as due to injection of deep CO2-rich
mafic magma into the shallow crustal plumbing system. More recent (post-1970), milder (VEI 1–2) eruptions,
instead, do only exhibit evidence for low-pressure (P b 50–60 MPa), volatile-poor (H2O b 0.3–1.7 wt%; CO2
b 23–308 μg/g) magmatic conditions. These are manifested as andesitic magmas, recording multiple magma
mixing events, in pyroxene inclusions.Wepropose that post-1970s eruptions are possibly related to the high viscosity
of resident magma in shallow plumbing system (b2.4 km), due to crystallization and degassing
Type
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