<p>The data from the Rosetta mission enabled the reconstruction of the shape of comet 67P/Churyumov-Gerasimenko (hereafter 67P) and the identification of the terrains and features forming its surface. The highly irregular &#160;shape of the comet poses a challenge for the depiction of these geological features on two-dimensional maps. Standard global map projections cannot display the complete surface of 67P because different points on the surface can have the same longitude and latitude.&#160; As a consequence, the geological maps published to date are&#160; created on top of comet images, making them dependent on the viewing angle and image coverage and resolution.</p><p>Here, we make use of the recently published Quincuncial Adaptive Closed Kohonen (QuACK) map. It projects the complete surface of 67P unambiguously onto a square. The QuACK map is topologically equivalent to the Peirce quincuncial projection of the world, which makes it&#160; possible to define generalized longitudes and latitudes. These can be used within any global map projection in order to obtain an&#160; unambiguous QuACK version.</p><p>The mapping of geological features is carried out in three dimensions employing the Small Body Mapping Tool (SBMT). We use images from&#160; the OSIRIS Narrow Angle Camera aboard Rosetta which have been projected onto the shape model of the SBMT. The three-dimensional coordinates are then projected onto two-dimensional maps, either in the QuACK map projection or in the QuACK version of&#160; the equidistant cylindrical projection. We present individual maps for 17 of the 26 regions of 67P, mostly located in the northern&#160; hemisphere. The new maps combine features published in previous studies with newly identified features.</p><p>We discuss the distribution of geological features and the characteristics of the regions. In order to align region boundaries with geological features, we propose two modifications of region definitions.</p>