We have investigated the trends in the formation of carbon vacancies in binary transition metal (TM) carbides using density functional calculations for two common TM carbide crystal structures, namely the B1 (rocksalt) and WC structure types. The TM are taken from group IV (Ti, Zr, Hf), V (V, Nb, Ta) and VI (Cr, Mo, W) of the periodic table, as well as Sc from group III. For B1-structured TM carbides, the general trend is that it is easier for C vacancies to be formed as the number of valence electrons in the system increases. The exception is ScC where C vacancies are rather easy to form. It is also clear that the formation of C vacancies depends on the growth conditions: For TM-rich conditions, B1-structured carbides will always favour C vacancy formation. For C-rich conditions it is energetically favourable to form C vacancies in ScC, VC, NbC, CrC, MoC and WC. Experimentally large C vacancy concentrations are found in B1-structured TM carbides and our calculations are in line with these observations. In fact, TiC, ZrC, HfC and TaC are the only B1-structured TM carbides that do not spontaneously favour C vacancies and then only for C-rich conditions. C vacancies may still be present in these systems, however, due to the high temperatures used when growing TM carbides. In the case of WC-structured TM carbides, C vacancy formation is not energetically favourable irrespective of the growth conditions, which is the reason why this structure is only found close to a one-toone metal-to-carbon ratio. In addition, we have investigated the change in the local structure induced by the presence of vacancies as well as the associated relaxation energy. We find that relaxations of the atoms close to the C vacancy is smaller in the WC-structured carbides than in B1-structured carbides. The smaller relaxations in WC-structured carbides works towards a lower tendency for C vacancies to be formed in the WC-structured than in B1-structured carbides since relaxations always work towards stabilising the vacancy.One striking feature of the TM carbides is that they are almost never found in ideal stoichiometry and often display large deviations from the ideal one-to-one metalto-carbon ratio. [1][2][3][4][5] The vacancy concentration in TiC can be as large as 50% 1 while still maintaining the rock-salt crystal structure and without any secondary Ti phase. This has, obviously, resulted in many investigations of the