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Polar Lunar Regions: Exploiting Natural and Augmented Thermal EnvironmentsIn polar regions of the Moon, some areas within craters are permanently shadowed from solar illumination and can reach temperatures of 100 K or less. These regions could serve as cold traps, capturing ice and other volatile compounds. These potential ice stores have many applications for lunar exploration. Within double-shaded craters, even colder regions exist, with temperatures never exceeding 50 K in many cases. Observed temperatures suggest that these regions could enable equivalent liquid nitrogen cryogenic functions. These permanently shaded polar craters also offer unprecedented high-vacuum cryogenic environments, which in their current state could support cryogenic applications. Besides ice stores, the unique conditions at the lunar poles harbor an environment that provides an opportunity to reduce the power, weight, and total mass that needs to be carried from the Earth to the Moon for lunar exploration and research. Reducing the heat flux of geothermal, black body radiation can have significant impacts on the achievable temperature. With a few manmade augmentations, permanently shaded craters located near the lunar poles achieve temperatures even lower than those that naturally exist. Our analysis reveals that lightweight thermal shielding within shaded craters could create an environment several Kelvin above absolute zero. The temperature ranges of both naturally shaded and thermally augmented craters could enable the long-term storage of most gases, low-temperature superconductors for large magnetic fields, devices and advanced high-speed computing instruments. Augmenting thermal conditions in these craters could then be used as a basis for the development of an advanced thermal management architecture that would support a wide variety of cryogenically based applications. Lunar exploration and habitation capabilities would significantly benefit if permanently shaded craters, augmented with thermal shielding, were used to facilitate the operation of near absolute zero instruments, including a wide variety of cryogenically based propulsion, energy, communication, sensing, and computing devices. The required burden of carrying massive life-supporting components from the Earth to the Moon for lunar exploration and research potentially could be reduced.
Document ID
20070032630
Acquisition Source
Stennis Space Center
Document Type
Conference Paper
Authors
Ryan, Robert E.
(Science Systems and Applications, Inc. Bay Saint Louis, MS, United States)
McKellip, Rodney
(NASA Stennis Space Center Stennis Space Center, MS, United States)
Brannon, David P.
(NASA Stennis Space Center Stennis Space Center, MS, United States)
Underwood, Lauren
(Science Systems and Applications, Inc. Bay Saint Louis, MS, United States)
Russell, Kristen J.
(Aerospace Corp. Chantilly, VA, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2007
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
SSTI-2220-0121
Meeting Information
Meeting: AGU 2007 Winter Meeting
Location: San Francisco, CA
Country: United States
Start Date: December 10, 2007
End Date: December 14, 2007
Sponsors: American Geophysical Union
Funding Number(s)
CONTRACT_GRANT: NNS04AB54T
Distribution Limits
Public
Copyright
Other

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