The knowledge of the universe future is of fundamental importance for any advanced civilization. We study the future of singular dark universe where thermal effects due to the Hawking radiation on the apparent horizon of the FRW universe are taken in consideration. It is shown that dark universe which ends up at finite-time Type I and Type III singularity or infinite-time Little Rip singularity transits to finite-time Type II singularity due to account of thermal effects. On the same time, the Type II and IV singular universe does not change its qualitative behavior. The combined account of quantum and thermal effects shows that depending on specific features of the universe only one of effects is dominant. When (conformal matter) quantum effects are dominant, the future singularity is usually removed while for dominant thermal effects the universe final state is the Type II singularity.

LaTeX, 11 pages, to appear in Physics of the Dark Universe