Structure and magnetic properties of nanocrystalline P6/mmm out-ofequilibrium precursors of hard magnetic R-3m Sm 2 (Fe,M) 17 C (M=Ga,Si,) and I4/mmm Sm(Fe,Co,Ti) 11 equilibrium phases, are presented. Their structure is explained with a model ground on the R 1−s T 5+2s formula (R=rare-earth, s=vacancy rate, T=transition metal) where s Sm atoms are statistically substituted by s transition metal pairs. The Rietveld analysis (RA) provides the stoichiometry of the precursors, 1:9 and 1:10, respectively precursor of 2:17 and 1:12 phases. The interpretation of the Mössbauer spectra of the 1:9 and 1:10 phases, is based on the correlation between δ and the Wigner-Seitz Cell volumes, calculated from the structural parameters. The δ behaviour of each crystallographic site versus Co content, defines the Co location while it confirms that of Si and Ga obtained by RA. Substitution occurs in 3 g site, whatever Co or M. The Sm(Fe,Co,Ti) 10 and Sm(Fe,M) 9 C Curie temperature (T c ) are compared to those of the equilibrium phases, the effects of Fe substitution and C addition are discussed. The maximum μ 0 H c is obtained for low M or Co content, for auto-coherent diffraction domain size ∼30 nm. SmFe 8.75 Ga 0.25 C and SmFe 8.75 Si 0.25 C with T c of 680 and 690 K, show respectively M r and μ 0 H c of 58 emu/g, 27 kOe and 95 emu/g, 15 kOe, values higher than those obtained for Sm 2 (Fe,M) 17 carbides.