In this paper, we report the relative SNe contributions on metal budget of ICM Abell 1837 galaxy cluster at redshift z $=$ 0.069. For purpose, analysed hot and obtained radial distributions by using XMM-Newton archival data with total exposure $\sim$100 ks. These measurements consist Mg, Si, S, Fe Ni within 0.7 R$_{500}$ radius which is divided into three concentric annuli. order to explain obs...