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The 31 brightest galaxies (m_B < 15 mag) inside the virial radius of theFornax cluster were observed from the centres to the outskirts with the MultiUnit Spectroscopic Explorer on the Very Large Telescope. These observationsprovide detailed high-resolution maps of the line-of-sight kinematics and linestrengths of the stars and ionised gas reaching 2-3 Re for 21 early-typegalaxies and 1-2 Re for 10 late-type galaxies. The majority of the galaxies areregular rotators, with eight hosting a kinematically distinct core. Only twogalaxies are slow rotators. The mean age, total metallicity, and [Mg/Fe]abundance ratio in the bright central region inside 0.5 Re and in the galaxyoutskirts are presented. Extended emission-line gas is detected in 13 galaxies,most of them are late-type objects with wide-spread star formation. Themeasured structural properties are analysed in relation to the galaxies'position in the projected phase space of the cluster. This shows that theFornax cluster appears to consist of three main groups of galaxies inside thevirial radius: the old core; a clump of galaxies, which is aligned with thelocal large-scale structure and was accreted soon after the formation of thecore; and a group of galaxies that fell in more recently.

The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps