A thermodynamic model recently developed by the authors considers martensit
ic iron-carbon alloys to be a mixture of body centred tetragonal Fe:C and b
ody centred cubic Fe:Va groups (Va = vacant interstitial site). In this inv
estigation, the model has been extended to multi-component carbon containin
g alloys. From thermodynamic T-o and experimental M-s temperatures of FeCr,
FeCrC, and FeMn alloys, driving forces were derived which were near 2100 J
/mol when plate martensite was formed, and proportional to the concentratio
n of the alloying elements when lath martensite was formed. Using the equat
ions describing the dependence of the driving forces on the concentration o
f alloying elements, a very good correspondence between M-s temperatures re
ported in TTT diagrams for alloys in the system FeCrMnC and calculated ones
was achieved. For FeNi alloys, T-o temperatures calculated by means of SGT
E data were at high Ni concentrations more negative than measured M-s tempe
ratures. By a fitting procedure, suitable solution parameters for the bcc p
hase were derived. Using these parameters, correct T-o and M-s temperatures
in binary FeNi as well as in FeCrNiC and FeNiC alloys were obtained.