Abstract. Methane (CH 4 ), 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 CH 4 to the atmosphere, although the biogeochemical processes involved in its formation are not fully understood. Several recent studies provided strong evidence of CH 4 production in oxic marine and freshwaters, but its source is still a topic of debate. Studies of CH 4 dynamics in surface waters of oceans and large lakes have concluded that pelagic CH 4 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 CH 4 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 CH 4 . Therefore, the coccolithophore Emiliania huxleyi was grown under controlled laboratory conditions and supplemented with two 13 C-labeled carbon substrates, namely bicarbonate and a position-specific 13 C-labeled methionine (R-S-13 CH 3 ). The CH 4 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 13 C-labeled substrate, the isotope label was observed in headspace CH 4 . Moreover, the absence of methanogenic archaea within the algal culture and the oxic conditions during CH 4 formation suggest that the widespread marine algae Emiliania huxleyi might contribute to the observed spatially and temporally restricted CH 4 oversaturation in ocean surface waters.