Evidence for methane production by the marine algae <i>Emiliania huxleyi</i>

Lenhart, K; Klintzsch, T; Langer, G; Nehrke, G; Bunge, M; Schnell, S; Keppler, F. 2016 Evidence for methane production by the marine algae <i>Emiliania huxleyi</i>. Biogeosciences, 13 (10). 3163-3174. 10.5194/bg-13-3163-2016

[img]
Preview
Text
bg-13-3163-2016.pdf - Published Version
Available under License Creative Commons Attribution.

Download (2MB) | Preview
[img] Other
bg-13-3163-2016.xml - Published Version
Available under License Creative Commons Attribution.

Download (187kB)
Official URL: http://dx.doi.org/10.5194/bg-13-3163-2016

Abstract/Summary

Methane (CH4), an important greenhouse gas that affects radiation balance and consequently the earth's climate, still has uncertainties in its sinks and sources. The world's oceans are considered to be a source of CH4 to the atmosphere, although the biogeochemical processes involved in its formation are not fully understood. Several recent studies provided strong evidence of CH4 production in oxic marine and freshwaters, but its source is still a topic of debate. Studies of CH4 dynamics in surface waters of oceans and large lakes have concluded that pelagic CH4 supersaturation cannot be sustained either by lateral inputs from littoral or benthic inputs alone. However, regional and temporal oversaturation of surface waters occurs frequently. This comprises the observation of a CH4 oversaturating state within the surface mixed layer, sometimes also termed the "oceanic methane paradox". In this study we considered marine algae as a possible direct source of CH4. Therefore, the coccolithophore Emiliania huxleyi was grown under controlled laboratory conditions and supplemented with two 13C-labeled carbon substrates, namely bicarbonate and a position-specific 13C-labeled methionine (R-S-13CH3). The CH4 production was 0.7 µg particular organic carbon (POC) g−1 d−1, or 30 ng g−1 POC h−1. After supplementation of the cultures with the 13C-labeled substrate, the isotope label was observed in headspace CH4. Moreover, the absence of methanogenic archaea within the algal culture and the oxic conditions during CH4 formation suggest that the widespread marine algae Emiliania huxleyi might contribute to the observed spatially and temporally restricted CH4 oversaturation in ocean surface waters.

Item Type: Publication - Article
Divisions: Marine Biological Association of the UK > Other (MBA)
Depositing User: Barbara Bultmann
Date made live: 03 Oct 2016 16:06
Last Modified: 06 Jun 2017 16:17
URI: http://plymsea.ac.uk/id/eprint/7232

Actions (login required)

View Item View Item