  We extend the method of Kerr/CFT correspondence recently proposed in
arXiv:0809.4266 [hep-th] to the extremal (charged) Kerr black hole embedded in
the five-dimensional G\"{o}del universe. With the aid of the central charges in
the Virasoro algebra and the Frolov-Thorne temperatures, together with the use
of the Cardy formula, we have obtained the microscopic entropies that precisely
agree with the ones macroscopically calculated by Bekenstein-Hawking area law.
