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Preliminary Analysis: Am-241 RHU/TEG Electric Power Source for NanosatellitesThe Februay 2013 Space Works Commercial report indicates a strong increase in nano/microsatellite (1-50 kg) launch demand globally in future years. Nanosatellites (NanoSats) are small spacecraft in the 1-10 kg range, which present a simple, low-cost option for developing quickly-deployable satellites. CubeSats, a special category of NanoSats, are even being considered for interplanetary missions. However, the small dimensions of CubeSats and the limited mass of the NanoSat class in general place limits of capability on their electrical power systems (especially where typical power sources such as solar panels are considered) and stored energy reserves; restricting the power budget and overall functionality. For example, leveraging NanoSat clusters for computationally intensive problems that are solved collectively becomes more challenging with power related restrictions on communication and data-processing. Further, interplanetary missions that would take NanoSats far from the sun, make the use of solar panels less effective as a power source as their required area would become quite large. To overcome these limitations, americium 241 (Am-241) has been suggested as a low power source option. The Idaho National Laboratory, Center for Space Nuclear Research reports that:  (Production) requires small quantities of isotope - 62.5 g of Pu-238; 250 g Am- 241 (for 5 We); Am-241 is available at around 1 kg/yr commercially; Am-241 produces 59 kev gammas which are stopped readily by tungsten so the radiation field is very low. Whereby, an Am-241 source could be placed in among the instruments and the waste heat used to heat the platform; and  amounts of isotope are so low that launch approval may be easier, especially with tungsten encapsulation. As further reported, Am-241 has a half-life that is approximately five times greater than that of Pu- 238 and it has been determined that the neutron yield of a 241-AmO(sub 2) source is approximately an order of magnitude lower than that of a 238-PuO(sub 2) source of equal mass and degree of (sup 16)O enrichment. Also it has been demonstrated that shielded heat sources fuelled by oxygen-enriched 238-PuO(sub 2) have masses that are up to 10 times greater than those fuelled by oxygenenriched 241-AmO(sub 2) with equivalent thermal power outputs and neutron dose rates at 1 m radii. For these reasons, Am-241 is well suited to missions that demand long duration electrical power output, such as deep spaceflight missions and similar missions that use radiation-hard electronics and instrumentation that are less susceptible to neutron radiation damage.
Document ID
20140008746
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Robertson, Glen A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Young, David
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Cunningham, Karen
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Kim, Tony
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ambrosi, Richard M.
(Leicester Univ. United Kingdom)
Williams, Hugo R.
(Leicester Univ. United Kingdom)
Date Acquired
July 7, 2014
Publication Date
February 24, 2014
Subject Category
Spacecraft Propulsion And Power
Report/Patent Number
M14-3212
Meeting Information
Meeting: Nuclear and Emerging Technologies for Space (NETS 2014)
Location: NASA Stennis Space Center, MS
Country: United States
Start Date: February 24, 2014
End Date: February 26, 2014
Sponsors: American Nuclear Society, Universities Space Research Association
Distribution Limits
Public
Copyright
Public Use Permitted.
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