Infrared astronomy is crucial for exploring the universe, but due to limitations in detector performance and the scarcity of suitable sites, China suffers from a severe shortage of astronomical observation equipment in the infrared band. Kunlun Station in Antarctica possesses unique natural conditions such as dryness, cold, and long polar nights, providing unparalleled advantages for near-infrared astronomical observations. However, it also faces challenges such as harsh environments, unmanned operation, limited energy, and snow and frost accumulation. This paper summarizes the advantages and challenges of near-infrared astronomical observation in Antarctica, the current status and plans for Antarctic infrared astronomy both domestically and internationally, and analyzes the key technologies of Antarctic infrared telescopes and existing technological accumulations (mainly including methods for suppressing radiation from the telescope itself and instruments, methods for de-icing mirrors, infrared detector technology, telescope control systems, and optimized dewar/cryostat design), providing technical references for the future development of Antarctic infrared telescopes.