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An Extension of Analysis of Solar-Heated Thermal Wadis to Support Extended-Duration Lunar Exploration

Author
Gokoglu, S. A.
Published
April 2010.
Physical Description
1 electronic document
Additional Creators
Balasubramaniam, R., Suzuki, N. H., Wegeng, R. S., and Sacksteder, K. R.
Online Version

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Summary
The realization of the renewed exploration of the Moon presents many technical challenges; among them is the survival of lunar surface assets during periods of darkness when the lunar environment is very cold. Thermal wadis are engineered sources of stored solar energy using modified lunar regolith as a thermal storage mass that can supply energy to protect lightweight robotic rovers or other assets during the lunar night. This paper describes an extension of an earlier analysis of performance of thermal wadis based on the known solar illumination of the Moon and estimates of producible thermal properties of modified lunar regolith. The current analysis has been performed for the lunar equatorial region and validates the formerly used 1-D model by comparison of predictions to those obtained from 2-D and 3-D computations. It includes the effects of a thin dust layer covering the surface of the wadi, and incorporating either water as a phase-change material or aluminum stakes as a high thermal conductivity material into the regolith. The calculations indicate that thermal wadis can provide the desired thermal energy and temperature control for the survival of rovers or other equipment during periods of darkness.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 20100015637.
NASA/TM-2010-216255.
AIAA Paper 2010-797.
E-17241.
48th Aerospace Sciences Meeting; 4-7 Jan. 2010; Orlando, FL; United States.
Terms of Use and Reproduction
Copyright, Distribution as joint owner in the copyright.
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