Collisional excitation of light hydrides is important to fully understand the complex chemical and physical processes of atmospheric and astrophysical environments. Here, we focus on the NH(X 3 Σ − )-Ar van der Waals system. First we have calculated a new three-dimensional Potential Energy Surface (PES), which explicitly includes the NH bond vibration. We have carried out the ab initio calculations of the PES employing the open-shell single-and double-excitation couple cluster method with non-iterative perturbational treatment of the triple excitations [RCCSD(T)]. To achieve a better accuracy, we have first obtained the energies using the augmented correlationconsistent aug-cc-pVXZ (X = T, Q, 5) basis sets and then, we have extrapolated the final values to the complete basis set limit. We have also studied the collisional excitation of NH(X 3 Σ − )-Ar at the close-coupling level, employing our new PES. We calculated collisional excitation cross sections of the fine-structure levels of NH by Ar for energies up to 3000 cm −1 . After thermal average of the cross sections we have then obtained the rate coefficients for temperatures up to 350 K. The propensity rules between the fine-structure levels are in good agreement with those of similar collisional systems, even though they are not as strong and pronounced as for lighter systems, such as NH-He. The final theoretical values are also compared with the few available experimental data.I.