The Present Paper Provides Solution of Bianchi Type- Iii Bulk Viscous String Cosmological Model of Assuming That (I) Ξ2 = Μ2θ and (Ii) Σ ∞ Θ Which Leads to Β = Γζ (Where Μ and Ζ Are Constants, Ζ Is Bulk Viscosity and Θ Is Scalar of Expansion). Various Physical and Geometrical Features of the Model Are Also Found and Discussed.