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Solid-State Power Generating Microdevices for Distributed Space System ArchitecturesDeep space missions have a strong need for compact, high power density, reliable and long life electrical power generation and storage under extreme temperature conditions. Conventional power generating devices become inefficient at very low temperatures (temperatures lower than 200 K encountered during Mars missions for example) and rechargeable energy storage devices cannot be operated thereby limiting mission duration. At elevated temperatures (for example for planned solar probe or Venus lander missions), thin film interdiffusion destroys electronic devices used for generating and storing power. Solar power generation strongly depends upon the light intensity, which falls rapidly in deep interplanetary missions (beyond 5 AU), and in planetary missions in the sun shadow or in dusty environments (Mars, for example). Radioisotope thermoelectric generators (RTGs) have been successfully used for a number of deep space missions RTGs. However, their energy conversion efficiency and specific power characteristics are quite low, and this technology has been limited to relatively large systems (more than 100 W). The National Aeronautics and Space Administration (NASA) and the Jet Propulsion Laboratory (JPL) have been planning the use of much smaller spacecrafts that will incorporate a variety of microdevices and miniature vehicles such as microdetectors, microsensors, and microrovers. Except for electrochemical batteries and solar cells, there are currently no available miniaturized power sources. Novel technologies that will function reliably over a long duration mission (ten years and over), in harsh environments (temperature, pressure, and atmosphere) must be developed to enable the success of future space missions. It is also expected that such micropower sources could have a wide range of terrestrial applications, in particular when the limited lifetime and environmental limitations of batteries are key factors. Additional information is contained in the original extended abstract.
Document ID
20010041230
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Fleurial, J.-P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Patel, J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Snyder, G. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Huang, C.-K.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Averback, R.
(Illinois Univ. Urbana, IL United States)
Hill, C.
(Illinois Univ. Urbana, IL United States)
Chen, G.
(California Univ. Los Angeles, CA United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Forum on Innovative Approaches to Outer Planetary Exploration 2001-2020
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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