Archive of News and Press Releases

PS101 - Weekly Report No. 3 | 26 September - 2 October 2016

Hot and Cold at Gakkel Ridge of the Central Arctic Basin

[04. October 2016] 

The third week of expedition PS101 was dedicated to the study of hydrothermal venting under the ice. The Arctic fall season has begun.

At great depths below the sea, new seafloor is formed as tectonic plates are spread apart. The tectonic and volcanic forces within such spreading zones form vast submarine ridge systems within all oceans.  The Gakkel Ridge of the Arctic Ocean is Earth’s slowest spreading mid-ocean ridge system with on average a centimeter of new ocean crust forming each year. It is also the least known ridge system, as it is ice covered virtually permanently and very hard to access – except for the research icebreaker Polarstern. It was thought that Gakkel Ridge is quite inactive, but recent research cruises have shown evidence for volcanism and hydrothermal venting.  This expedition aims to study the origin of the spectacular seamounts found along Gakkel Ridge, and how they influence ocean currents and Arctic life (Fig. 1).

For our second working area after the Karasik seamount, we selected a small, steep and rocky mound of 8 km diameter, which shows evidence of active hydrothermalism. The mount rises more than 1000 m from the rift valley and appears to have recently been volcanically active, as evidenced by the vast occurrence of fresh pillow basalts and glass shards near its summit. We were able to map the area precisely using the ships own Multibeam Echosounder, an ATLAS Hydrosweep system. Common echosounders such as those used for fishing or as a depth sensor use only one beam of sound for imaging. But this one has 960 individual beams to record the shape of the seafloor below the ship across a wide angle. The lower figures show a 3D view as seen from the northwest and a profile view between each of the sites. This bathymetric data is then used for further exploration and sampling of the seafloor (Fig. 2).

With the OFOS’ (Ocean Floor Observatory System) first dive, we land in the middle of an otherworldly landscape of piles of broken basalt blocks. But on our way up to the peak of the mound, we encounter rather fresh pillow lava strands, which looks like they have recently been squeezed out, only to freeze up in the ice-cold Arctic deep-sea bottom waters. Some of the rocks that we find in the vicinity of the peak of the mound show glassy surfaces, indicating their recent origin (Fig. 3).  Volcanism supplies heat from the Earth’s interior that provides energy for hydrothermal activity. Where the cold ocean water comes into contact with the hot rocks deep within the Earth, chemical reactions produce a variety of energy rich gases which escape through fissures and chimneys to the seafloor and overlying waters – a real witches brew of hot vent fluids.

Already during the first dive, we discovered hydrothermal precipitates and potential seepage sites at the seafloor near the summit of the volcano (Fig. 4). The type of hydrothermalism present at the seafloor depends primarily on the amount of heat available and the types of rock percolated by the fluids. Currently, we are looking for the main vents of the mound, which produce the characteristic plumes of energy-rich substances and particles above the mound. If we find them, then their specific morphology, the color of the chimneys and the fluids emanating, as well as the types of life associated with the vent structures will tell us more about the underlying geology and chemistry of the ongoing hydrothermalism at Gakkel Ridge.

To search for the hydrothermal vent plumes, the characteristic signature of hot, energy and particle rich fluids emitted from distinct sources at the seafloor, the oceanographers apply a technique known as a “tow-yo” survey. During a tow-yo, the CTD is towed by the ship, while simultaneously being raised and lowered through the water column using the ship’s winch. In this way, the vertical and horizontal distribution of potential plume signals in temperature, turbidity and redox-potential can be mapped. But how can we do that in ice-covered seas? We use the passive drift of the ice instead of actively towing, which would require ice-breaking.  The first attempt to catch the plume was not so lucky: the icedrift was not cooperating and carried us away from our target site.  But with the second attempt, we had much better luck and found the first indication of active venting in the form of a particle plume, accompanied by a warm temperature anomaly above the mount at a water depth of 2600m, 300-500 m above the peak (Fig. 5). All sensors show anomalies in measured values when compared to the values of background deep-sea waters: the small volume of vent fluid mixed upwards from the vents can be detected by temperature and turbidity sensors on the water sampler, and in sensors measuring for chemical redox potential. What is called “plume” or “vent smoke” cannot be seen by the naked eye, but our first samples made the chemists on board and at home very happy: we have abundant methane, hydrogen and silicate in the plume waters. We continue to dive with OFOS right under the plume, equipped with the very same sensors and see similar signals on several terraces with outcroppings of orange rocks.

But what could cause such signatures in the plume? One possibility is that the vent-source on the seafloor is not a typical “black smoker” in which sulfide minerals precipitate as soon as the hot vents erupt into the ocean at around 350-400°C.  In such a case, both the turbidity signals and the redox signals coincide.  Instead, we observe an absence of particles within waters with the strongest chemical anomalies, and then increasing turbidity in waters as the plume disperses, suggesting that the particles are actively forming in the dispersing plume. In this case, any polymetallic sulfides would be expected to have precipitated beneath the seafloor before the vents erupt. The colder (300°C) clear fluids, enriched in dissolved iron as well as methane and other gases would then rise up through the water column, and only as the plume disperses and continues to mix with the oxygen-rich seawater would the dissolved Fe begin to react to form iron oxide “rust” particles.  We are therefore keeping our eyes open for chimneys emitting hot clear fluids from the seafloor, more reminiscent of an underwater fire-hydrant than a black smoker.

Molecular hydrogen and methane are major reduced compounds emitted from hydrothermal vents. To quantify these potential microbial energy sources, their concentrations were determined from water samples retrieved in different water sampler casts with on board gas chromatographs. The fresh plume has very high hydrogen and methane concentrations with up to 350 nM hydrogen and 280 nM of methane indicating that there are several mM of these compounds in the source vent fluids. Notably, the ratios of hydrogen and methane are highly variable in different plume samples. This indicates that the individual plumes may derive from different venting sources with substantially different chemistry. Alternatively, this variability may reflect different preferences of the microorganisms for the plume gases.  Previous studies have shown that hydrogen consumption in plumes is more rapid than methane oxidation, thus ‘older’ plumes may have more methane remaining than hydrogen. To determine whether the kinetics of microbial hydrogen and methane oxidation are due to different affinities by microorganisms, incubations with natural plume microbial communities have been started by the microbiologists on board. Reduced compounds of the plume waters may provide an energy source for chemosynthetic bacteria, which can fix CO2 just like plants, but without sunlight. First results show that the microbial activity in the plume waters is much higher than in control experiments conducted with water collected from reference sites, distant from the hydrothermal waters. We additionally have a novel spectrometric device on board that lets us take a first glimpse on the origin of the methane. It is isotopically much heavier than the atmospheric methane, suggesting that it is formed by abiotic processes in the seabed.

In the coming weeks, we will go forth and back between our young, hot mound and the old, cold large Karasik Seamount in the attempt to further integrate our different research aims, tasks and get the most out of our diverse range of scientific instrumentation. As an even cooler refreshment, we plan a sea ice station every 2-3 days. Also the under-ice robot NUI has started its scientific diving activity first in Automated Underwater Vehicle (AUV) mode, and has already produced 2 high-resolution bathymetry maps and one survey for a high resolution photomosaic of the seafloor. It really is a very special combination of extreme environment research when half of the scientists stare at the strange lava rocks and unknown deep-sea life thousands of meters under the ice, whilst the other half of the team drills ice-cores, places sea-ice buoys and measures the characteristics of the seasonal freeze-up process. Around us, the Arctic fall has begun, and it is dark, foggy and often very cold outside with temperatures of -10°C or even below. So all of us are equally happy about relaxing from time to time in the cozy belly of the ship, equipped as it is with relaxing meeting rooms, a gym, sauna and table tennis facilities – the focus of an ongoing tournament involving both scientists and the skilled ships crew. We have just celebrated the midpoint of the cruise, with a reception on the ice, and a very nice BBQ. Half of the mission is over, and we have still so many Gakkel Ridge mysteries to solve. Please cross your fingers for luck with ice, wind and weather out here.  

All participants are in good health and are sending greetings to families, friends and colleagues.

Antje Boetius

Contact

Science

Annabel Ledrich
+49(471)4831-2268
Annabel.Ledrich@awi.de

Scientific Coordination

Rainer Knust
+49(471)4831-1709
Rainer Knust

Assistant

Sanne Bochert
+49(471)4831-1859
Sanne Bochert