Understanding the genesis and evolution of the universe can be accomplished by studying binary systems. We were able to locate and offer an analysis of the geometrical and physical properties of HIP 70868 through this investigation. Tokovinin’s orbital solution method and AlWardat’s spectral analysis method both helped us achieve this. We constructed a modified orbit for the system using Tokovinin’s formula and determined its mass to be Mdyn = 2.72 ± 0.20 M⊙. We were able to create a spectral energy distribution and validate the system’s physical parameters using AlWardat’s Method. We were able to determine the spectral types of the system’s components, S.T.A. F8/G0 and S.T.B. G0, as well as the masses of the components, which were determined to be M=MA + MB = 2.9 ± 0.3 M⊙. This demonstrates the accuracy of the techniques employed. Additionally, we proposed a new parallax measurement, π =13.64 mas, which perfectly aligns the two approaches.