Carbon, nitrogen, and noble gas isotopes reveal deep volatile signatures in thermal springs in the Central Volcanic Zone (CVZ) of the Andes
Peter H. Barry, J. de Moor, Michael W. Broadley, Alan Seltzer, D.V. Bekaert, Karthikeya Patil, CGE Bartels, Edward Young, Brett E. Longworth, Bernardo Barosa, Alessia Bastianoni, Deborah Bastoni, Martina Cascone, Susan Turner, Rebecca Tyne, Molly Anderson, Kan Li, Joshua Curtice, Nitish Kumar, Gerdhard L Jessen, Jenny M. Blamey, Carlos Ramírez, Agostina Chiodi, Felipe Aguilera, Susanna Layana, Cristóbal González, Ana M. Aguilera, GPJ Masías Alvarez, Bernard Marty, Karen G. Lloyd, Donato Giovannelli
Abstract
• Carbon, noble gases and clumped N 2 isotopes data from thermal springs in the Central Volcanic Zone of the Andes suggest a dominantly crustal source of volatile elements. • Thermal spring samples with non-atmospheric He-Ne characteristics have low radiocarbon activities, indicating that dissolved carbon (available for use by microbes in the deep biosphere) is deeply derived and likely old (>22,000 years). • High precision Xe isotopes suggest a similar amount of crustal and mantle Xe as suggested independently by He isotopes, pointing to the coupled release of crustal volatiles by bulk degassing of the crust via melting. • Clumped N 2 results suggest essentially no air-derived N 2 and that crustal N 2 can be released at high temperatures in addition to magmatic N 2 . In subduction zones, thermal springs release deeply-sourced volatiles from Earth's mantle, crust, and/or subducted slab-derived material. The origin and apparent ages of these volatiles are important for understanding the deep volatile cycle, which in turn affects the distribution of microbial life in the subsurface. Here, we report carbon ( 13 C, 14 C), noble gas (He, Ne, Ar, Kr and Xe), and clumped nitrogen isotope data in gas and water samples from thermal springs within the Central Volcanic Zone (CVZ) of the Andean Convergent Margin (ACM). He isotopes show that CVZ gases are predominantly sourced from the crust (∼77 %), with smaller mantle contributions (∼23 %), consistent with previous studies from the CVZ. Thermal spring samples with non-atmospheric He-Ne characteristics have low 14 C activities, and are deeply derived (i.e., from the mantle and crust) and old (>22,000 years). To gain additional constraints on volatile sources, a gas sample from Pirquitas Argentina was analyzed using a new high-precision technique to reveal significant geogenic anomalies in argon ( 40 Ar/ 36 Ar = 492), fissiogenic xenon (88 % crustal), and helium (84 % crustal) isotopes. Clumped N 2 isotopologue results also indicate that the N 2 -rich Pirquitas sample is dominated by crustal and magmatic N 2 , which was unambiguously released at high temperatures (indicated by Δ 30 of ∼0‰). When taken together, all carbon, noble gas and clumped N 2 isotope data from CVZ thermal springs point toward a predominantly crustal source of volatile elements, which is consistent with the thick crust beneath the arc. We conclude that thermal springs with noble gas isotopic evidence for minimal air contributions are old, suggesting that any microbial communities entrained in them are also supported by deeply-derived and old organic carbon.