General comments
The manuscript by Schnabel et al. presents an impressive set of pore-water data and sulfate reduction rates as well as metagenomic and metascriptomic data for 50 (40?) sediment cores/gravity cores retrieved from the SW Barents Sea shelf. The objectives of the study are to assess how the magnitude of upward methane/hydrocarbon flux impacts the geochemistry, biogeochemical processes – namely microbial sulfate reduction - and microbial communities in the surface and subsurface sediments.
The manuscript is definitely of interest for the readers of Biogeosciences and generally well-written. However, there are several issues that need to be specified and described much more precisely – in particular the terms „seepage“ and „HC reservoir“. There are also several statements and concepts presented in the manuscript that are not correct as given (e.g. statements about seismics). The authors should definitely define the term „seepage“ and say what they mean when they speak of „seepage“. What about the activity/episodicity of any potential seepage? Please, precisely specify and distinguish whether you speak of transport of methane by molecular diffusion (as is obviously the case at most of your sites) or fluid seepage – i.e. migration of fluids and or free gas bubbles through the pore space of the sediments at rates exceeding those of molecular diffusion. In other words, if upward methane transport occurs in the form of molecular diffusion – as seems to be the case at most of your study sites – I would not speak of seepage. I would therefore suggest to more generally speak of upward methane „fluxes“ throughout the manuscript. The different intensities/magnitudes of methane upward flux then determine the depth position of the SMT and the magnitude of SR as well as the type of microbial community/ies.
I also did not fully understand which type of „HC reservoir“ precisely you speak of. This is also not clear from Chapter 2. Do you mean free gas in the deeper subsurface? What about gas hydrates? The potential role of the presence of gas hydrates in the subsurface – as an intermediate methane reservouir - has not been mentioned and discussed at all. There are numerous studies that have demonstrated that during active seepage events methane is transported upwards from deeper sources (mostly in the form of free gas) and becomes trapped in the form of gas hydrates at shallower sediment depth (if positioned within the gas hydrate stability zone). After these gas hydrate deposits have formed they give off methane, which diffuses upward towards the sediment surface and leads to the establishment of an SMT where AOM consumes most of the upward diffusing methane (e.g., Dickens, 2001, GCA; Lapham et al., 2010, EPSL). The methane gradient – thus magnitude of upward flux – and depth position oft he SMT then depends on the depth position of the gas hydrates.
Moreover, the referencing to previous relevant studies is also not sufficient. In the past 20 to 25 years numerous studies have been performed to investigate the regional variability of upward methane fluxes. There are for example several studies by the group of Gerald Dickens that have investigated differences in upward methane fluxes – for example on Blake Ridge and in other ocean areas. Also the impact that upward methane fluxes and in particular of AOM on the geochemical composition of pore waters and sediments – including mineral dissolution (e.g. magnetite) and precipitation of authigenic minerals – including carbonates, barite, Fe sulfides/rock magnetic properties is mostly missing (see suggestions given below). There are also several previous studies that have correlated pore-water profiles with micobial communities (e.g. Oni et al., 2005, Frontiers Microbiol.; Wunder et al., 2021, ISME; Schnakenberg et al., 2021, Frontiers Microbiol.).
It would also be good to have a zoom-in map of the study area in order to have an idea of the bathymetry and seafloor topography. The insert shown given in Fig. 1 b is not very informative. It would be good to see seafloor topography/bathymetry in ordert o assess whether there are typical seep seafloor features of methane seepage such as pockmarks and to find out at which water depth the study sites are located (also with respect to judging whether the sites lie within the gas hydrate stability or not).
Specific comments
L. 24 and throughout the manuscript: The term „inconspicuous“ is rather unusual in this context. Do you mean „low“ upward fluxes?
L. 30 Do you mean constant/no depletion instead of „linear“
L. 40: What precisely do you mean with „inconspicuous HC seepage“ ? I would rather speak of low methane „fluxes“. i.e. diffusive flux.
L. 41: „shallower“ than what precisely?!
L. 46: What precisely is a „minor“ seep ?
L. 48: The effect of upward diffusion of methane and resulting AOM on sediment geochemistry has been shown and reported by numerous studies: including Riedinger et al. – and Henkel et al. etc.
Ls. 49 to 51: These sentences are unclear. What precisely is a „distal manifestation“? „seabed“? I guess you mean sediment surface, right?!
L. 52: I guess you mean „geochemical“ instead of geological, right?!
L. 54 ff.: The statement – as it stands here – is not correct. It is not methane-containing fluids that produce seismic signals but the presence of free gas that induces an impedance contrast that is registered by seismics. Fluids of high dissolved methane concertrations are not detectable by seismic approaches. Please, rephrase this more precisely throughout the manuscript.
L. 58 ff.: Strictly speaking, it is not the flux of methane itself but the consumption of methane/HCs in the process of AOM that impacts the geochemical composition of pore-waters and sediments. This has already been demonstrated by numerous studies, some of which should definitely also be refered to/cited here. So, in addition to what you describe/refer to in this part of the introduction you should at leasdt also mention a few of the most prominent impacts of upward methane flux and the resulting oxidation of methane by sulfate (AOM) . namely the precipitation of authigenic carbonates and barite (e.g. studies by Bohrmann, Torres, etc.) and also the dissolution of magnetite producing distinct minima in magnetic susceptibility (e.g. Riedinger et al., 2005; März et al., 2008).
L. 62/63: I also do not agree with this statement …. Methane formation is extremely widespread in continental margin sediments – and in most cases is not associated with underlying HC reservoirs but rather formed in situ by biogenic processes.
L. 70: This is not entirely true … rather depends where you are. There are also more recent studies on the role of sulfate reduction (e.g. Bowles et al., 2014).
L. 90: Please, also give reference to other relevant previous studies – e.g. Niewöhner et al. (1998; GCA), Treude et al.; Riedinger et al. (2005, 2014, 2017), März et al. (2008), Henkel et al. (2012; GCA).
L. 113: This statement contradicts that in the abstract. Here you speak of 40 gravity cores while in the Abstract you mention 50 gravity cores.
Figure 1: The zoom-in in Fig 1b is not informative at all. It would be good to have a map showing the bathymetry/seafloor topography. The map also does not indicate where the potential „HC reservoirs“ are found in the deeper subsurface.
Figure 2 is very difficult to read and understand. What precisely is shown in Figs, 2a to 2d? These are definitely not measured pore-water profiles … are these modelled profiles or gradients? Please, specify and overhaul this figure as well as the figure caption.
The title of this figure says „sulfite“ ?! I guess you mean sulfide, correct?! |