  The Fornax galaxy cluster is an ideal nearby laboratory in which to study the
impact of dense environments on the evolution of galaxies. The Fornax3D survey
offers extended and deep integral-field spectroscopic observations for the
brightest 33 galaxies within of virial radius of the Fornax cluster, obtained
with the MUSE integral-field spectrograph, mounted on Unit Telescope 4 (Yepun)
of ESO's Very Large Telescope in Chile. The Fornax3D data allowed us to
reconstruct the formation of early-type galaxies in the cluster and to explore
the link with spiral galaxies. Results have been published in 19 refereed
papers since 2018. In this paper we review the broad goals of this campaign,
its main results and the potential for future studies combining the MUSE data
with the abundant multi-wavelength data coverage for Fornax.
