EGU26-10762, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-10762
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 05 May, 15:15–15:25 (CEST)
 
Room -2.21
Mercury emission from the Tajogaite eruption La Palma, Canary Islands
Eduardo Lodoso1,2, Nemesio M. Pérez1,2, Gladys V. Melián1,2, Beverley C. Coldwell1,2, Óscar Perdomo-Sosa1,2, Pedro A. Hernández1,2, María Asensio-Ramos1, Eleazar Padrón1,2, and Germán D Padilla1,2
Eduardo Lodoso et al.
  • 1Instituto Volcanológico de Canarias, (elodoso2503@iter.es)
  • 2Instituto Tecnológico y de Energías Renovables (ITER), 38600 Granadilla de Abona, Tenerife, Canary Islands

Mercury (Hg) is a volatile and highly toxic metal released into the environment from both natural and anthropogenic sources. Volcanic activity represents one of the major primary natural contributors to atmospheric Hg, with previous estimates of global annual volcanic emissions ranging from approximately 50 to 700 t·a-1 (e.g., Nriagu and Becker, 2003; Pyle and Mather, 2003). The main sources of uncertainty of the total emission of volcanic Hg are rooted in a lack of measurements from volcanic eruptions, due to the logistical challenges of collecting gaseous Hg samples from actively erupting plumes. One potential method to quantify volcanic Hg emission from eruptions is through the analysis of Hg adsorbed to the surface of volcanic ash particles, which can readily be sampled on the ground downwind of eruptions.

The purpose of this study is to estimate mercury emissions from the 2021 Tajogaite eruption at Cumbre Vieja volcano (La Palma, Canary Islands), a record-breaking event characterized by exceptionally high volatile output, with CO2 and SO2 emissions of 28 ± 14 Mt (Burton et al., 2023) and 1.6 ± 0.1 Mt (Esse et al., 2025), respectively.

Mercury degassing during the Tajogaite eruption was estimated using Hg/SO2 molar ratios derived from sulphate (SO42-) concentrations in ash leachates and mercury content in dried volcanic ash samples. Volcanic ash from the eruption was collected almost daily at five monitoring stations located at varying distances from the vents. Sulphate and Hg analyses were performed via ion chromatography and mercury-specific atomic absorption spectrometry (AAS-Hg) using a RA-915 Mercury Analyzer. In terms of analytical performance, an adequate linear factor adjustment (R2= 0.99) and linear range (0.3-30 ng Hg) were achieved for the quantification of Hg in ash samples.

The average sulphate concentration in the ash leachates was 3.49 × 104 µg·kg⁻¹, ranging from 1.21 × 104 to 8.48 × 104 µg·kg⁻¹, while the average Hg content in the dried ash was 1.69 × 103 µg·kg⁻¹, ranging from 0.28 × 103 to 9.40 × 103 µg·kg⁻¹. These measurements yield an estimated average Hg/SO2 molar ratio of 1.55 × 10-5, with a range from 0.76 × 10-5 to 3.54 × 10-5. Considering an SO2 emission of 1.6 Mt from the Tajogaite eruption, the corresponding estimated mercury emission is 77.6 t on average, with a range of 3.8 to 177 t.

References
Burton, M., Aiuppa, A., Allard, P. et al. (2023). Exceptional eruptive CO2 emissions from intra-plate alkaline magmatism in the Canary volcanic archipelago. Commun. Earth Environ. 4, 467. https://doi.org/10.1038/s43247-023-01103-x

Esse, B., Burton, M., Hayer, C. et al. (2025). Forecasting the evolution of the 2021 Tajogaite eruption, La Palma, with TROPOMI/PlumeTraj-derived SO2 emission rates. Bull. Volcanol. 87, 20,  https://doi.org/10.1007/s00445-025-01803-6

Nriagu, J. and Becker, C. (2003). Volcanic emissions of mercury to the atmosphere: global and regional inventories. Sci. Total Environ. 304, 3–12.
Pyle, D.M. and Mather, T.A. (2003). The importance of volcanic emissions for the global atmospheric mercury cycle. Atmos. Environ. 37, 5115–5124.

How to cite: Lodoso, E., Pérez, N. M., Melián, G. V., Coldwell, B. C., Perdomo-Sosa, Ó., Hernández, P. A., Asensio-Ramos, M., Padrón, E., and Padilla, G. D.: Mercury emission from the Tajogaite eruption La Palma, Canary Islands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10762, https://doi.org/10.5194/egusphere-egu26-10762, 2026.