The pure rotational spectrum of FeN in its X 2 D i ground state has been recorded using millimeter-wave direct absorption techniques in the range 198-525 GHz. New measurements have also been carried out for FeC (X 3 D i ), in particular of the fine-structure component and the 54 FeC isotopomer. These molecules were created by Q p 1 the reaction of iron vapor with either CH 4 (FeC) or N 2 (FeN) in a DC discharge. Eight rotational transitions were recorded for FeN in its lowest-lying spin component, , and multiple transitions were measured for FeC Q p 5/2 in all three of its spin-orbit ladders, as well as for . These data have been analyzed, and precise 54 FeC (Q p 3) spectroscopic constants for both radicals have been determined. The fine structure in FeC was found to exhibit an irregular pattern, indicating that higher order spin-orbit perturbations are occurring in this molecule. Although only one spin component was observed for FeN, the bond length established from the data is consistent Q p 5/2 with a 2 D ground state, as indicated by theory. Fe-bearing species are relevant to many astrophysical topics, including astrochemistry, dust grains composition, nucleosynthesis, and mass loss from asymptotic giant branch stars.