  Recently, there has been much attention devoted to resolving the quantum
corrections to the Bekenstein-Hawking (black hole) entropy, which relates the
entropy to the cross-sectional area of the black hole horizon. Using
generalized uncertainty principle (GUP), corrections to the geometric entropy
and thermodynamics of black hole will be introduced. The impact of GUP on the
entropy near the horizon of three types of black holes; Schwarzschild,
Garfinkle-Horowitz-Strominger and Reissner-Nordstr\"om is determined. It is
found that the logarithmic divergence in the entropy-area relation turns to be
positive. The entropy $S$, which is assumed to be related to horizon's
two-dimensional area, gets an additional terms, for instance $2\, \sqrt{\pi}\,
\alpha\, \sqrt{S}$, where $\alpha$ is the GUP parameter.
