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The Drake Passage is an oceanic gateway of about 850 km width located between South America and the Antarctic Peninsula that connects the southeastern Pacific Ocean with the southwestern Atlantic Ocean. It is an important gateway for mantle flow, oceanographic water masses, and migrations of biota. This sector developed within the framework of the geodynamic evolution of the Scotia Arc, including continental fragmentation processes and oceanic crust creation, since the oblique divergence of the South American plate to the north and the Antarctic plate to the south started in the Eocene. As a consequence of its complex tectonic evolution and subsequent submarine processes, as sedimentary infill and erosion mainly controlled by bottom currents and active tectonics, this region shows a varied physiography. We present a detailed map of the bathymetry and geological setting of the Drake Passage that is mainly founded on a new compilation of precise multibeam bathymetric data obtained on 120 cruises between 1992 and 2015, resulting in a new Digital Bathymetric Model with 200 × 200 m cell spacing. The map covers an area of 1,465,000 km2 between parallels 52°S and 63°S and meridians 70°W and 50°W at scale 1:1,600,000 allowing the identification of the main seafloor features. In addition, the map includes useful geological information related to magnetism, seismicity and tectonics. This work constitutes an international cooperative effort and is part of the International Bathymetric Chart of the Southern Ocean project, under the Scientific Committee on Antarctic Research umbrella. © 2018, © 2018 The Author(s). Published by Informa UK Limited, trading as Taylor & Francis Group on behalf of Journal of Map., This work was supported through projects CTM2014-60451-C2-02/01, CTM2017-89711-C2-2/1-P and special action CTM2011-13970-E from ?Ministerio de Ciencia, Innovaci?n y Universidades? of Spain. This study is part of the British Antarctic Survey Polar Science for Planet Earth Programme funded by the Natural Environment Research Council. This work was also supported by the Scientific Committee on Antarctic Research. We thank to the crew and technicians of the RRS James Clark Ross, BIO Hesp?rides, RV Polarstern, RVIB Nathaniel B. Palmer, and the RV Araon and RV Onnuri for their support and cooperation in obtaining these data under sometimes severe sea conditions. The Scientific Committee on Antarctic Research (SCAR) is acknowledged for providing the framework that allowed this broad international venture. The production of the map was supported by SCAR.

IX Congreso Geológico de España, Huelva, Septiembre 2016, The Drake Passage is an oceanic gateway of about 850 km width located between South America and the Antarctic Peninsula that connects the southeastern Pacific and the southwestern Atlantic oceans and is an important gateway for mantle flow, oceanographic water masses, and migrations of biota. This gateway developed within the framework of geological evolution of the Scotia Arc. As a consequence of this and subsequent submarine processes, this region shows a varied physiography. The new detailed map in the Drake Passage region is mainly founded on a compilation of precise multibeam bathymetric data obtained on cruises between 1992 and 2014, and covers the area between parallels 52ºS and 63ºS and meridians 70ºW and 50ºW. The new map that we present is based in a DTM with 200 m cell resolution of the seafloor in Drake Passage that permits identification of the main seafloor features and the map includes additional useful geological information. This work constitutes an international cooperative effort and is part of IBCSO project (International Bathymetric Chart of the Southern Ocean), under the SCAR umbrella., Instituto Geológico y Minero de España, España, British Antarctic Survey, Reino Unido, Departamento de Geodinámica, Universidad de Granada, España, Instituto Andaluz de Ciencias de la Tierra, Consejo Superior de Investigaciones Científicas, España, Instituto Andaluz de Ciencias de la Tierra, Universidad de Granada, España, Jet Propulsion Laboratory M/S 300-323, Estados Unidos, Alfred Wegener Institute, Alemania, Korea Polar Research Institute, Corea, Departamento de Geología y Geoquímica, Universidad Autónoma de Madrid, España, Lamont-Doherty Earth Observatory, Columbia University, Estados Unidos