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The 15 January 2022 Hunga (Tonga) eruption: A gas-driven climactic explosion

dc.contributor.authorHenley, Richard W.en
dc.contributor.authorde Ronde, Cornel E.J.en
dc.contributor.authorArculus, Richard J.en
dc.contributor.authorHughes, Grahamen
dc.contributor.authorPham, Thanh Sonen
dc.contributor.authorCasas, Ana S.en
dc.contributor.authorTitov, Vasilyen
dc.contributor.authorWalker, Sharon L.en
dc.date.accessioned2025-12-16T01:38:01Z
dc.date.available2025-12-16T01:38:01Z
dc.date.issued2024en
dc.description.abstractAn extraordinarily powerful, explosive eruption occurred from Hunga volcano in the Tonga island arc on 15 January 2022 and generated an eruption column 58 km high. The explosive eruption also generated atmospheric gravity waves, extreme runup tsunamis and quite unusual and destructive meteotsunamis. Together these place this VEI 6 eruption as, globally, one of the largest of the past 300 years. Based on the oceanic context of Hunga volcano, it has previously been assumed that the eruption was phreatomagmatic through a fuel-coolant Surtseyan-type interaction, but this is not supported by satellite imagery. Similarly, it has been suggested that a caldera-collapse was the eruption trigger, but this is not supported by bathymetric data or the seismicity recorded during the eruption. Here we develop a new model based on the observed energetics and time sequence of the eruption integrated with understanding of the internal structure of active volcanoes and their characteristic high flux discharges of volcanic gas. It has been shown elsewhere that magma-derived reactive gases (H2O, CO2, SO2, HCl, etc) aggressively alter the volcanic rocks in the core of a volcano leading to self-sealing of gas flow to the surface and consequent changes to deviatoric stress in the structure. Common minerals developed by these reactions include anhydrite (CaSO4), sulphides and silica (quartz), all of which have been recorded in volcanic ejecta including at Hunga. We here develop a first order numerical model that quantifies how the free discharge of such gas to the surface may progressively become choked by these sealing reactions leading to increased internal gas pressure. Hydraulic fracture of the seal occurs when the transmitted pressure of the compressed magmatic gas beneath the seal increases to a value greater than the lithostatic pressure plus the tensile strength of the sealed rock. This initiates the explosive release of compressed gas whose high-power discharge progressively develops and enlarges a crater. At the same time, the explosion feeds upon itself by generating larger pressure gradients in the pressurized gas within the fractured porous rock mass of the core of the volcano. Excavation of the crater may intersect high level intrusions and produce the pumice rafts that were observed after the eruption. The eruption itself diminished in intensity as the gas pressure in the reservoir declined. At Hunga, the eruption excavated an 850 m deep, 2-3 km diameter steep-walled crater. This volume may be assumed to approximate the volume of fractured porous rock (the control volume of the eruption) whose trapped gas was mined by the eruption until surrounding gas pressure was depleted. Our numerical model shows that the calculated potential energy of the trapped compressed gas matches the independent observations of the scale of the eruption. Sensor data have since shown that gas bubble flares continued for at least 6 months after the eruption indicating continued depletion of the gas reservoir of rocks surrounding the new crater. The systems-based, gas-driven model for the Hunga climactic eruption developed here also applies to Plinean-type eruptions on subaerial arc volcanoes such as at Pinatubo (Philippines) 1991.en
dc.description.sponsorshipCornell de Ronde reports financial support was provided by New Zealand Strategic Science Investment Fund. If there are other authors, they declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.As researchers we acknowledge that climactic eruptions cause major loss of homes and lives so that we hope continued exploration of their causes may help to mitigate future risk in many parts of the world. Richard Henley wishes to thank the Australian Academy of Sciences for encouragement and the provision of an opportunity to present this interpretation of the 2022 Tonga eruption: https://www.science.org.au/news-and-events/events/haddon-forrester-king-lecture-by-professor-richard-henley. We especially thank Steve Ingebritsen and Tobias Fischer for constructive review comments. We also thank Steven F. Cox and Fred J. Prata for useful discussions during the initial development of this paper. Thomas Donda is thanked for assistance with graphics. Cornell de Ronde acknowledges support from the New Zealand Strategic Science Investment Fund (SSIF). Thanh-Son Pham and Ana Casas Ramos, respectively, acknowledge financial support from the Australian Research Council through a Discovery Early Career Researcher Award (DE230100025) and Discovery Project Grant (DP200100406). This paper has been assigned a PMEL contribution number of 5570.en
dc.description.statusPeer-revieweden
dc.format.extent14en
dc.identifier.issn0377-0273en
dc.identifier.otherORCID:/0000-0003-3202-1052/work/187191993en
dc.identifier.otherORCID:/0000-0001-5013-1701/work/187192921en
dc.identifier.otherORCID:/0000-0002-9057-4416/work/193550754en
dc.identifier.scopus85193227076en
dc.identifier.urihttps://hdl.handle.net/1885/733795295
dc.language.isoenen
dc.provenanceThis is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).en
dc.rights© 2024 The Authors. Published by Elsevier B.V. en
dc.sourceJournal of Volcanology and Geothermal Researchen
dc.subjectAtmospheric gravity wavesen
dc.subjectGas-solid reactionen
dc.subjectHydraulic fractureen
dc.subjectMagmatic vaporen
dc.subjectMeteotsunamisen
dc.subjectPlinean eruptionen
dc.titleThe 15 January 2022 Hunga (Tonga) eruption: A gas-driven climactic explosionen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage14en
local.bibliographicCitation.startpage1en
local.contributor.affiliationHenley, Richard W.; Department of Materials Physics, Research School of Physics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationde Ronde, Cornel E.J.; GNS Scienceen
local.contributor.affiliationArculus, Richard J.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationHughes, Graham; Department of Civil and Environmental Engineeringen
local.contributor.affiliationPham, Thanh Son; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationCasas, Ana S.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationTitov, Vasily; National Oceanic and Atmospheric Administrationen
local.contributor.affiliationWalker, Sharon L.; National Oceanic and Atmospheric Administrationen
local.identifier.citationvolume451en
local.identifier.doi10.1016/j.jvolgeores.2024.108077en
local.identifier.purec1e7637c-8f8f-4e74-bc74-6cf452ecfa43en
local.identifier.urlhttps://www.scopus.com/pages/publications/85193227076en
local.type.statusPublisheden

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