EGU24-22422, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-22422
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Temporal variations of sinking particulate organic radiocarbon in the deep Sargasso Sea

Charlotte Schnepper1, Rut Pedrosa-Pamies2, Maureen Conte2,3, Nicolas Gruber4, Negar Haghipour1,5, and Timothy Ian Eglinton1
Charlotte Schnepper et al.
  • 1Department of Earth Sciences, Geological Institute, ETH Zürich, Switzerland
  • 2Bermuda Institute of Ocean Sciences, St. Georges, Bermuda
  • 3Ecosystems Center, Marine Biological Laboratory, Woods Hole, MA, USA
  • 4Department of Environmental System Sciences, Institute of Biogeochemistry and Pollutant Dynamics, ETH Zürich, Switzerland
  • 5Laboratory of Ion Beam Physics, ETH Zürich, Zurich, Switzerland

The imprint of bomb radiocarbon on sinking particulate organic carbon (PO¹⁴C) intercepted by sediment traps, together with flux and elemental data, provides information about the origin and dynamics of oceanic particles (Hwang et al., 2010). Of particular interest is the question of the degree to which sinking POC in the deep ocean stems from overlying primary production, i.e., vertical supply via the biological pump, versus other processes such as advection and subsequent aggregation of resuspended sedimentary carbon originating from continental margins and other distal sources (Conte et al., 2019). In this context, natural abundance variations in 14C serves as a useful tracer given contrasting signatures recently fixed and pre-aged carbon sources. To quantify the seasonal to inter-annual variability in sinking PO¹⁴C, we have analyzed sediment trap samples from the Oceanic Flux Program (OFP) in the Sargasso Sea, a deep ocean time-series which has examined the particle flux and its composition at 500, 1500 and 3200 m water depths since 1978.

Radiocarbon measurements of POC of all OFP samples spanning September 2012 to December 2015 reveal seasonal and subseasonal variations in sinking PO¹⁴C with an amplitude in Δ¹⁴C values of ca. 100 ‰. This variability in Δ¹⁴C values is inversely linearly correlated with the proportion of lithogenic material to POC (LM:POC; r2=4.2, p <0.01). This relationship suggests that POC with high Δ¹⁴C values and a low LM:POC ratio reflect the supply of particles that sink vertically via the biological pump. Conversely, lower Δ¹⁴C values and high LM:POC ratios indicate laterally transported materials originating from resuspended sediments containing pre-aged organic carbon. Significant deviations from the linear regression (p <0.01) correlate with δ13C values, indicating an increased state of POC remineralization that is independent of Δ¹⁴C variations attributable to particle provenance.  

Over the 3.3 year period of observation, POΔ¹⁴C decreased by ca. 26 %, exceeding the expected annual decline (~6 ‰) based on reconstructed surface DI14C. This decline potentially could be linked to different source(s) of laterally supplied aged organic carbon associated with lithogenic material and/or a shift in the POΔ¹⁴C of the overlying flux (e.g.  from reduction in particle sinking speeds, enhanced decomposition, increased incorporation of aged suspended particles and/or dissolved organic carbon into the sinking flux). On-going work extending the OFP time-series will examine these multiyear trends and assess potential variability in the balance between vertically exported and laterally supplied POC to the deep ocean flux in the deep Sargasso Sea, enabling a better understanding of the underlying processes which control POC dynamics. 

How to cite: Schnepper, C., Pedrosa-Pamies, R., Conte, M., Gruber, N., Haghipour, N., and Eglinton, T. I.: Temporal variations of sinking particulate organic radiocarbon in the deep Sargasso Sea, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-22422, https://doi.org/10.5194/egusphere-egu24-22422, 2024.