We present precise values of the dipole polarizabilities () of the ground and metastable $\rm [4f^{14} 5d] ~ ^2D_{3/2}^+$, that are %vital {\bf important} in reducing systematics in the clock frequency of the $\rm[4f^{14}6s] ~ ^2S_{1/2} \rightarrow [4f^{14}5d] ~ ^2D_{3/2}\alpha\rm [4f^{14} 5d] ~ ^2D_{3/2}9.8(1) \times 10^{-40} ,,\rm Jm^2V^{-2}17.6(5) \times 10^{-40},, \rm Jm^2V^{-2}\rm [4f^{14} 5d] ~ ^2D_{3/2}- 12.3(3) \times 10^{-40},, \rm Jm^2V^{-2}-13.6(2.2) \times 10^{-40},,\rm Jm^2V^{-2}$. This corresponds to the differential scalar polarizability value of the above transition as (5)$,\times, 10^{-40},\rm Jm^2 V^{-2}-6.9,\times, 10^{-40}\rm Jm^2V^{-2}$. This results in the black-body radiation (BBR) shift of the clock transition as Hz at the room temperature, which is large as compared to the previously estimated values. Using the dynamic values, we report the tune-out and magic wavelengths that could be of interest to subdue %major systematics due to the Stark shifts and for constructing lattice optical clock using Yb.

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