4. Conclusions
A theoretical model was developed for the thermal efficiency predication of a Stirling cycle applied for lunar surface nuclear power system. It was found that the maximum of the thermal effi- ciency of about 0.29 could be obtained, when the hot side temperature was 1050 K. The radiation heat loss of the hot heat pipes could lead to the decrease of the thermal efficiency if the hot side temperature was higher. A decrease of the cold side temperature could result in an increase of the thermal efficiency. But lower cold side temperature would have bad effect on heat rejection to the outer space by radiation, which could lead to a larger system size and mass. When the cold side temperature was 500 K, the lowest mass of the power system of 6.6 ton can be obtained. Higher nominal convection heat transfer coefficient of the heat exchangers could improve the system thermal efficiency. A compromise between heat exchangers’ mass and system thermal efficiency should be considered, since higher values of nominal convection heat transfer coefficient of the heat exchangers resulted in a negligible increase of the thermal efficiency. In the future, more detailed description about the heat exchangers, Stirling engines and heat rejection system should be revealed.