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Hybrid star is the term given to a neutron star with a quark core. Due to alot of uncertainties in the calculations and compositions of such ahigh-density system, it is of great interest and a preferred scenario forparticle physicists and astrophysicists. To explore some novel aspects withinthe framework of the $5\mathcal{D}$ Einstein-Gauss-Bonnet(EGB) gravity, ourcurrent study presents a hybrid star model that includes strange quark matterin addition to regular baryonic matter. In hybrid stellar objects, a hadronicouter component surrounds a quark inner component, which prompts theconsideration of the most basic MIT bag model equation of state to correlatethe density and pressure of strange quark matter within the stellar interior,while radial pressure and matter density due to baryonic matter are connectedby a linear equation of state. The model is constructed within thespecifications of the Krori and Barua (KB) {\em ansatz} (Krori and Barua, J.Phys. A: Math. Gen. $\bold{8},508, 1975$). Here we present the solution for aparticular compact object 4U 1538 - 52 with mass $\mathcal{M} = 0.87 \pm0.07~\mathcal{M}_{\odot}$ and radius $\mathfrak{R} = 7.866_{-0.21}^{+0.21}$ km.We examine the fundamental physical characteristics of the star, whichhighlights how the values of matter variables are affected by the Gauss-Bonnetcoupling parameter $\alpha$. Finally, as it meets all the physical requirementsfor a realistic model, we have come to realize that our present model isrealistic.

Celestial attributes of Hybrid star in $5\mathcal{D}$ Einstein-Gauss-Bonnet gravity