Practical implementation of hybrid perovskite solar cells (PSCs) depends on achieving decent lifetimes under realistic operational conditions. The degradation pathways in PSCs are effectively mitigated using charge-transport interlayers, which are usually designed based on empiric considerations. Herein, we present a systematic comparative study of a series of hole-transport materials for p−i−n perovskite solar cells such as CuI, CuSCN, MnS, CuO x , MoO x , VO x , WO x , and PTAA and reveal their influence on the light-induced degradation of MAPbI 3 as a model perovskite absorber material. Using a set of complementary techniques, we demonstrate that WO x enables the best stack stability, while CuO x , on the contrary, strongly facilitates the degradation of the perovskite material due to the formation of PbO and other aging products. Furthermore, we show that such materials as CuO x , CuI, and CuSCN undergo severe intermixing with the deposited above perovskite absorber and, hence, could not form efficient hole-extraction layers in p−i−n perovskite solar cells. The obtained results provide important guidelines for the rational design of hole-transport materials for perovskite solar cells and feature the most promising candidates, which could enable the long-term operational stability of PSCs.