Open AccessTracking Formation of a Lava Lake From Ground and Space: Masaya Volcano (Nicaragua), 2014–2017
Author(s) -
Aiuppa Alessandro,
de Moor J. Maarten,
Arellano Santiago,
Coppola Diego,
Francofonte Vincenzo,
Galle Bo,
Giudice Gaetano,
Liuzzo Marco,
Mendoza Elvis,
Saballos Armando,
Tamburello Giancarlo,
Battaglia Angelo,
Bitetto Marcello,
Gurrieri Sergio,
Laiolo Marco,
Mastrolia Andrea,
Moretti Roberto
Publication year - 2018
Publication title -
geochemistry, geophysics, geosystems
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.928
H-Index - 136
ISSN - 1525-2027
DOI - 10.1002/2017gc007227
Subject(s) - lava , geology , volcano , magma , impact crater , plume , geochemistry , panache , lava dome , petrology , flux (metallurgy) , volcanic gases , fumarole , geomorphology , mineralogy , astrobiology , meteorology , chemistry , physics , organic chemistry
A vigorously degassing lava lake appeared inside the Santiago pit crater of Masaya volcano (Nicaragua) in December 2015, after years of degassing with no (or minor) incandescence. Here we present an unprecedented‐long (3 years) and continuous volcanic gas record that instrumentally characterizes the (re)activation of the lava lake. Our results show that, before appearance of the lake, the volcanic gas plume composition became unusually CO 2 rich, as testified by high CO 2 /SO 2 ratios (mean: 12.2 ± 6.3) and low H 2 O/CO 2 ratios (mean: 2.3 ± 1.3). The volcanic CO 2 flux also peaked in November 2015 (mean: 81.3 ± 40.6 kg/s; maximum: 247 kg/s). Using results of magma degassing models and budgets, we interpret this elevated CO 2 degassing as sourced by degassing of a volatile‐rich fast‐overturning (3.6–5.2 m 3 s −1 ) magma, supplying CO 2 ‐rich gas bubbles from minimum equivalent depths of 0.36–1.4 km. We propose this elevated gas bubble supply destabilized the shallow (<1 km) Masaya magma reservoir, leading to upward migration of vesicular (buoyant) resident magma, and ultimately to (re)formation of the lava lake. At onset of lava lake activity on 11 December 2015 (constrained by satellite‐based MODIS thermal observations), the gas emissions transitioned to more SO 2 ‐rich composition, and the SO 2 flux increased by a factor ∼40% (11.4 ± 5.2 kg/s) relative to background degassing (8.0 kg/s), confirming faster than normal (4.4 versus ∼3 m 3 s −1 ) shallow magma convection. Based on thermal energy records, we estimate that only ∼0.8 of the 4.4 m 3 s −1 of magma actually reached the surface to manifest into a convecting lava lake, suggesting inefficient transport of magma in the near‐surface plumbing system.