  We study the quasinormal modes of $p$-form fields in spherical black holes in
$D$-dimensions. Using the spherical symmetry of the black holes and gauge
symmetry, we show the $p$-form field can be expressed in terms of the coexact
$p$-form and the coexact $(p-1)$-form on the sphere $S^{D-2}$. These variables
allow us to find the master equations. By utilizing the S-deformation method,
we explicitly show the stability of $p$-form fields in the spherical black hole
spacetime. Moreover, using the WKB approximation, we calculate the quasinormal
modes of the $p$-form fields in $D(\leq10)$-dimensions.
