Abstract
Marine dissolved organic matter (DOM) is one of the largest reservoirs of reduced carbon on Earth. In the dark ocean (>200 m), most of this carbon is refractory DOM. This refractory DOM, largely produced during microbial mineralization of organic matter, includes humic-like substances generated in situ and detectable by fluorescence spectroscopy. Here we show two ubiquitous humic-like fluorophores with turnover times of 435±41 and 610±55 years, which persist significantly longer than the ~350 years that the dark global ocean takes to renew. In parallel, decay of a tyrosine-like fluorophore with a turnover time of 379±103 years is also detected. We propose the use of DOM fluorescence to study the cycling of resistant DOM that is preserved at centennial timescales and could represent a mechanism of carbon sequestration (humic-like fraction) and the decaying DOM injected into the dark global ocean, where it decreases at centennial timescales (tyrosine-like fraction).
Highlights
Marine dissolved organic matter (DOM) is one of the largest reservoirs of reduced carbon on Earth
The water mass composition of each water sample was described through the mixing of prescribed water types (WT) with a multi-parameter analysis
We identified 22 WT with 12 of them representing 90% of the total volume of water samples collected during the global cruise (Fig. 2)
Summary
Marine dissolved organic matter (DOM) is one of the largest reservoirs of reduced carbon on Earth. The dark global ocean appears to be a sink for fluorescent tyrosine-like (C4) component and has a turnover time of 379±103 years that is comparable to turnover time of DOC pool (estimated in 370 years[11]).
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