- INGV
In recent years, many studies have been devoted to quantifying and mapping terrestrial CO2 degassing. Besides climate effects, another reason to study the natural degassing of endogenous CO2 concerns its role in tectonics, and here I will focus primarily on this aspect, referring to the results obtained in central and southern Italy. In central and southern Italy, non-volcanic CO2 of deep origin is released from numerous vents and diffuse emission zones, and from groundwater with high CO2 content. Groundwater degassing was estimated coupling hydrogeochemical and hydrogeological data and using the mass balance of the carbon dissolved in the springs of high flow rate (hundreds to thousands kg/s). This approach allowed us both to quantify the emission (2.1 × 1011 mol yr−1) and to create a detailed map of the process. The map shows two large degassing structures: TRDS (Tuscan Roman degassing structure) and CDS (Campanian degassing structure). The same CO2-rich groundwater are “slightly thermal” having a temperature of few degree C higher than that expected for normal groundwater. These anomalous temperatures are due to high geothermal heat fluxes (up to 350 mW/m2). This coincidence, combined with the presence at depths > 10 km of a large zone of low-velocity of the seismic waves, suggested that the hot CO2-rich fluids are probably emitted from a large magmatic intrusion located in the root of the central Apennines. The Apennine belt is characterized by seismicity that recently peaked with strong earthquakes in 2009 (L'Aquila earthquake, M = 6.3) and 2016 (Amatrice-Norcia earthquakes, M = 6.0 and 6.5). We observed that CO2 emissions correlate with seismicity both geographically and over time: Apennine seismicity affects in fact the eastern edges of the TRDS and the CDS, and CO2 emissions increased during, and likely before, the 2009 and 2016 events.
How to cite: Chiodini, G.: Carbon dioxide earth degassing, heat flux and earthquakes in central and southern Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5052, https://doi.org/10.5194/egusphere-egu26-5052, 2026.