  We present the complete set of physical and geometrical parameters of the
visual close binary system GJ\,9830 for the first time by using Al-Wardat's
complex method. This method combines magnitude difference from speckle
interferometry, synthetic spectral energy distributions of the binary
components which are constructed depending on grids of Kurucz blanketed models
(Atlas9), along with the orbital solution by using Tokovinin's dynamical method
to estimate the parameters of the individual components. The analysis of the
system by using synthetic photometry resulted in the following set of
parameters: $T_{\rm eff.}=6220\pm 100$ \,K, $\rm log~g=4.30\pm 0.12$,
$R=1.10\pm0.08\,R_\odot$ for the primary component and $T_{\rm eff.}=4870\pm
100$\,K, $\rm log~g=4.60\pm 0.11$, $R=0.709\pm0.07\,R_\odot$ for the secondary
component. The recently published dynamical parallax from \textit{Gaia} space
mission was used to calculate the total mass of the binary system as
$1.75\pm0.06\, \mathcal{M}_\odot$ which coincides with those estimated by using
Al-Wardat's method as $ \mathcal{M}^{A}=1.18\pm0.10\, \mathcal{M}_\odot$, $
\mathcal{M}^{B}=0.75\pm0.08\, \mathcal{M}_\odot$.
  The analysis of the system reveals that both components belong to main
sequence stars with an age around $1.4\pm0.50$\,Gyr. The evolutionary tracks
and isochrones of the system's components are discussed, and the fragmentation
process is suggested as the most likely process for the formation of the
system.
