An investigation into the relative stabilities and equations of state of st
oichiometric FeS was conducted using first-principles pseudopotential calcu
lations. These calculations were based on density functional theory and per
formed using ultrasoft Vanderbilt pseudopotentials within the generalized g
radient approximation. We have identified four stable polymorphs of FeS alo
ng the 0 K isotherm as a function of pressure: troilite, an orthorhombic Mn
P-type structure, a monoclinic structure, and a CsCl-type structure. The ca
lculated internal energy as a function of volume for each polymorph was fit
ted to 4(th) order logarithmic and 3(rd) order Birch-Murnaghan equations of
state, yielding values for the bulk modulus, K, and its first and second d
erivatives with respect to pressure, K' and K ". These equations of state m
ay be used to characterize models of planetary cores.