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Title: 8th symposium on space nuclear power systems

Conference ·
OSTI ID:5626287

Tests were carried out to assess the impact of wind blown dust accumulation and abrasion on radiator surfaces on Mars. High emittance arc-textured copper and niobium-1 percent-zirconium samples were subjected to basaltic dust laden wind at Martian pressure (1000 Pa) at speeds varying from 19 to 97 m/s in the Martian Surface Wind Tunnel. The effect of accumulated dust was also observed by pre-dusting some of the samples before the test. Radiator degradation was determined by measuring the change in the emittance after dust was deposited and/or removed. The principle mode of degradation was abrasion. Arc textured Nb-1 percent-Zr proved to be more susceptible to degradation than Cu, and pre-dusting appeared to have lessened the abrasion.

Research Organization:
National Aeronautics and Space Administration, Cleveland, OH (USA). Lewis Research Center
OSTI ID:
5626287
Report Number(s):
N-91-20204; NASA-TM-103704; E-5841; NAS-1.15:103704; CONF-910116-; CNN: NCC3-19
Resource Relation:
Conference: 8. symposium on space nuclear power systems, Albuquerque, NM (USA), 6-10 Jan 1991; Other Information: Sponsored by NASA, New Mexico Univ., Strategic Defense Initiative Organization, DOE, and the AF
Country of Publication:
United States
Language:
English