EGU26-20443, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-20443
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 10:45–12:30 (CEST), Display time Monday, 04 May, 08:30–12:30
 
Hall X2, X2.25
The Serracozzo cave, Etna Volcano, Italy: A peculiar cavity developed during the 1971 flank eruption within an eruptive fissure and an arterial lava flow
Danilo Cavallaro1, Sonia Calvari1, Gaetano Giudice1, Danilo Messina1, Stephen Self2, Giuseppe Puglisi1, Emanuela De Beni1, Massimo Cantarero1, Daniele Morgavi3, and Roberto Maugeri1
Danilo Cavallaro et al.
  • 1INGV, Osservatorio Etneo, Italy (danilo.cavallaro@ingv.it)
  • 2Earth & Planetary Science, University of California, Berkeley, CA 94702, USA
  • 3Department of Earth Sciences (DiSTAR), University Federico II, Complesso Universitario di Monte Sant'Angelo (Ed. 10), Via Vicinale Cupa Cintia 21, 80126, Napoli, (Italy).

The Serracozzo cave is one of the most famous and fascinating lava tubes of Etna volcano. The cave formed in about one month during the final phase of the well-known 1971 flank eruption. It is a morphologically complex volcanic cavity because of its dual-nature: the upper section developed directly within the eruptive fissure, while the lower part formed within a ravine by sealing of an arterial ‘a‘ā lava flow, resulting in a distinctive lava tube. The features of the cavity formed within the eruptive fissure reveal a pulsating emplacement of the feeder dike, with alternation of magma pressure build-up and release. The dike emplaced a structural weakness along the Etna’s NE flank, which was frequently intruded by several other dikes during previous historical lateral eruptions. During its way to the surface the dike progressed by pulses, expanding laterally and then upwards. The same pulses occurred during its propagation down slope, where we observed wide chambers alternated to narrow passages. The effusive vents at the top of the fissure became skylights that acted as pressure release valves, forming short pāhoehoe overflows around the vents with upper level cavities partially merging with the main one during lava drain back. To characterize the volcanic features of the cave and reconstruct its spatiotemporal evolution, we conducted a traditional geological field survey integrated with old photos taken during the eruption, historical topographic maps and previous field surveys. Furthermore, high-resolution digital models of both the internal and external environments were generated using Terrestrial Laser Scanning (TLS) and Unoccupied Aerial Systems (UAS). This study realized with a multi-proxy approach is extremely valuable for hazard assessment because it allows us to constrain the timing necessary for the development and growth of the internal and external lava tube features and of how they evolved with time.

How to cite: Cavallaro, D., Calvari, S., Giudice, G., Messina, D., Self, S., Puglisi, G., De Beni, E., Cantarero, M., Morgavi, D., and Maugeri, R.: The Serracozzo cave, Etna Volcano, Italy: A peculiar cavity developed during the 1971 flank eruption within an eruptive fissure and an arterial lava flow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20443, https://doi.org/10.5194/egusphere-egu26-20443, 2026.