Biological assemblages of three new mud volcanoes along deep-reaching transform...

• Author(s): Cunha, M. ; Hilário, Ana ; Vieira, R.P. ; Adão, H. ; Aranda, Silva A. ; Ravara, A. ; Terrinha, P. ; Hensen, C.
• Date: 2012
• Persistent ID: http://hdl.handle.net/10174/7244
• Origin: Repositório Científico da Universidade de Évora
• Subject(s): Mud volcanos; Biological assemblages; Horseshoe Abyssal Plain (NE Atlantic)
• Document Type: Lecture
• Language: English

Description

Previous work on the Gulf of Cadiz (S Iberian Margin) has revealed several mud volcanoes sitting on the accretionary wedge and aligned along west-east trending transform faults. The source of fluids in these mud volcanoes is several kilometres below the seafloor and their geochemical composition indicates that they are affected, in different degrees, by oceanic crust alteration, implying that there is active flow connecting the oceanic basement and the seafloor. To date, such kind of hydrothermal circulation is only known for relatively young oceanic crust (<60 Ma) and therefore the existence of a hydrological connection between old, sedimented oceanic crust and the seafloor is a phenomenon that may represent a (missing) link between hydrothermal vents at mid-ocean ridges and cold seeps at continental margins. During the research cruise M86/5 on board RV Meteor within the research program of SWIMGLO (PTDC/MAR/100522/2008), selected sites along the westward trending transform faults of the adjacent Horseshoe Abyssal Plain were investigated and three new mud volcanoes, Michael Ivanov, Abzu and Tiamat were discovered at ca. 4500m depths. Initial findings showed the occurrence of chemosymbiotic metazoan hosts (Acharax gadirae and several Frenulata species) and a high diversity in meiofauna and macrofauna. Nematodes were abundant followed by copepods and polychaetes but tanaids, amphipods, polychaetes and bivalves (Nuculanidae) were also well represented. An AUV survey further enabled to map the distribution of Frenulata fields, bivalve shells and disturbed sediment patches on the crater of Michael Ivanov MV. The results are discussed in relation to previous knowledge on the Gulf of Cadiz seeps.