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NASA Technical Reports Server (NTRS) 20070010457: Survey of Dust Issues for Lunar Seals and the RESOLVE Project PDF

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Preview NASA Technical Reports Server (NTRS) 20070010457: Survey of Dust Issues for Lunar Seals and the RESOLVE Project

“Survey of Dust Issues for Lunar Seals and the RESOLVE Project” By Margaret P. Proctor and Paula Dempsey Abstract Lunar dust poses a technical challenge for sealing applications on the moon. A survey of seals used in Apollo lunar missions is presented as well as lunar soil characteristics and a description of the lunar environment. Seal requirements and technical challenges for the volatiles characterization oven and hydrogen reduction reaction chamber of the RESOLVE project are discussed. The purpose of the RESOLVE project is to find water or ice in lunar soil and demonstrate the ability to produce water, and hence oxygen and hydrogen, from lunar regolith for life support and propellants. 1 v o g . a s a n . w h w p w c n o a h r s s y B k al e r s s o e p t W n n S m e o r e ar ct e n si t m D o i n e n e v u oj a mp Di Ce st 06 y L l r u 0 r P a Co es ch e S 2 H o P h r ues f OLVE y and nical ructur esear d at t ary Ai 4-15, nd, O s S B r a St R e d 1 a s E to ch n nt n er el I R c e d n e o b v t o n s c e s e r M a e e e m l u P l C D th P. he als A G Pr al/S ove of d t ri S e N n t f e e o A S n y a t atio e ar m a N A r M nist v g a S dmi ur ar e A A T e S M N c a s Sp l 6 d a 0 n a e s 0 c S uti 2 a n o r e A al n o ati N 2 v o s g d ch or asa. e u t n g m c w. n a n w o s f o w ol i al s iti n pr 5 es nt e e os atio e to h 200 ctiviti nme thos urfac dep r g c a o n s e o n r ir a m at Expl challe on.” aut Ma urface to env ger th st fro elimin nar nical e Mo tron nar s osed e lon rties e du e or s e v h h u p d z s and Space Administration Challenges of Future Lu st represents the single largest tec human presence on t Harrison Schmidtt, Apollo 17 A he extent and duration of planned l gher than prior Apollo experiences. ystems and components will be ex r periods of time orders of magnitu eviously addressed. mitigation strategies: esign systems tolerant of dust prop evelop techniques to clean or remo ctive abatement methods to minimi nd/or adhesion of dust autic Du T hi S fo pr st D D A a n u ero “ D 1. 2. 3. 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Primarily non-toxic Not active in vacuum Highly charged <20 μm high ferromagneti -4 o1.72-2.95 x 10W/cm K 0.3 (compression index) Protection for Environmental Cos of the Lunar Materials Technol t g r sn u i a Dd e n )e ) 2c m ) 9o on u c y se 19Pr nautics and Space Administrati L haracteristic ze hape ulk Density (0-30 ardness orosity (0-15 cm) ohesion (0-15 cm) oxicity orrosiveness ectrostatic agnetic hermal Conductivit ompressibility (loo nce: Fuhs, S., Harris, J.(he Lunar Environment. ero C Si S B H P C T C El M T C ret A e al ef n R o ati N

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