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The goal of this survey is to study the formation and evolution of the MilkyWay halo to deduce its assembly history and the 3D distribution of mass in theMilky Way. The combination of multi-band photometry, Gaia proper motion andparallax data, and radial velocities and the metallicity and elementalabundances obtained from low-resolution spectra of halo giants with 4MOST, willyield an unprecedented characterisation of the Milky Way halo and its interfacewith the thick disc. The survey will produce a volume- and magnitude-limitedcomplete sample of giant stars in the halo. It will cover at least 10,000square degrees of high Galactic latitude, and measure line-of-sight velocitieswith a precision of 1-2 km/s as well as metallicities to within 0.2 dex.

4MOST Consortium Survey 1: The Milky Way Halo Low-Resolution Survey