Mantle-derived helium and carbon in groundwaters and gases of Mount Etna, Italy

Details Mantle-derived helium and carbon in groundwaters and gases of Mount Etna, Italy Mantle-derived helium and carbon in groundwaters and gases of Mount Etna, Italy

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997e%26psl.148..501a&link_type=abstract

Earth and Planetary Science Letters, Volume 148, Issue 3-4, p. 501-516.

Computer Science

32

Scientific paper

We report the first detailed investigation of both helium and carbon isotopes in groundwaters and gases of Mt. Etna, providing new insight into the distribution, origin and budget of magmatic gas release at this very active volcano. A mantle-derived magmatic component, with ultimate 3He/(4He) ratio of 6.9 +/- 0.2 Ra and δ13C of about -4‰, is identified in both types of fluids, depending on their location and the extent of their dilution by either air (gases) or a mixture of dissolved air and organic carbon (waters). Apart from the summit zone, this magmatic component is preferentially concentrated in CO2-rich groundwaters that issue from two remote sectors of the south-southwest and eastern volcano flanks, where its proportion increases with the altitude of meteoric recharge (or the length of pathflow) of the waters. Such a pattern suggests that, in addition to possible local gas input, the groundwaters collect much of their dissolved magmatic He and C while they infiltrate and flow through one of the more elevated, gas-effusing parts of the volcanic pile, among which the south-southeast fracture zone of Etna is the best candidate. These observations provide a new framework for remote geochemical monitoring of the volcano. The 3He/(4He) ratio of the magmatic gas end-member coincides with that of helium trapped in the He-rich olivine crystals of Etna basalts (mean range: 6.7 +/- 0.4 Ra), pointing to its negligible dilution by radiogenic He from the crustal basement and further constraining the 3He/(4He) ratio of the present-day Etna magma. While being lower than the typical MORB value of 8 Ra, this ratio is the highest for an active volcano in continental Europe and probably tracks a relatively radiogenic upper mantle zone that is upwelling beneath this region. The estimated outputs of mantle-derived CO2 and 3He from Etna account for 10% and 15%, respectively, of estimates for global subaerial volcanic emissions. This huge contribution results from continuous degassing of mostly unerupted He- and C-rich alkaline basaltic magma, which occurs principally through the central open conduits and secondarily through the flanks of the volcano. Groundwaters carry only a minor fraction (~ 3%) of total emitted CO2 and 3He.

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