  The perfect physical and geometrical parameters of the main-sequence close
visual binary system (CVBS), HIP\,105947, are explicitly presented. These
parameters have been constructed conclusively using Al-Wardat's complex method
for analyzing CVBSs, which is a method for constructing a synthetic spectral
energy distribution (SED) for the entire binary system using individual SED for
each component star. Which in its turn built using Kurucz
({\fontfamily{cmtt}\selectfont ATLAS9}) line-blanketed plane-parallel models.
At the same time, the orbital parameters for the system are calculated using
Tokovinin's dynamical method for constructing the best orbits of the
interferometric binary system. Henceforth, the mass-sum of the components, the
$\triangle\theta $ and $\triangle\rho $ residuals for the system are
introduced. The combination of Al-Wardat's and Tokovinin's methods yields the
estimation of the physical and geometrical parameters to their best values. The
positions of the components of the system on the evolutionary tracks and
isochrones are plotted, and their formation and evolution are discussed.
