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Performance Evaluation of a Vapor-compression-cycle Based Heat Pump System for a Lunar Habitat under the Impact of Dust Deposits on the Coupled Radiators
- Source :
- Acta Astronautica. 194
- Publication Year :
- 2022
- Publisher :
- United States: NASA Center for Aerospace Information (CASI), 2022.
-
Abstract
- Space exploration gains new momentum. A near goal is set by NASA to return humans to the Moon andestablish a sustainable presence on the lunar surface for more repeatable and affordable expeditions.The lunar dust is one of the dangerous environment hazard causing serious problems for explorationactivities. In this paper, in order to study the impact of lunar dust on the performance of a thermalmanagement system for a lunar habitat, a dynamical model of an active thermal control system that iscomprised of a vapor-compression cycle heat pump and a radiator loop is developed. A heat pump to liftthe heat rejection temperature is required due to high lunar daytime surface temperature. Parametricstudies on radiator size, percentage of dust coverage on the radiator, and lunar habitat location arecarried out. The results show that lunar deposits can significantly increase the power consumption ofthe thermal management system. A dust covered radiator panel results in net heat input to the heattransfer fluid during the period of strong solar irradiance, causing deteriorated performance of theradiator loop. The lunar dust contamination problem raises the requirement of redundancy design of asystem for fault tolerance. A synergetic design of a thermal management system, a power generationsystem and robotic maintenance system is proposed to achieve maximal mass cut for a whole lunarhabitat system.
- Subjects :
- Lunar And Planetary Science And Exploration
Subjects
Details
- Language :
- English
- ISSN :
- 00945765
- Volume :
- 194
- Database :
- NASA Technical Reports
- Journal :
- Acta Astronautica
- Notes :
- 80NSSC19K1076
- Publication Type :
- Report
- Accession number :
- edsnas.20220008035
- Document Type :
- Report
- Full Text :
- https://doi.org/10.1016/j.actaastro.2022.01.040