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Structural Design Considerations for a 50 kW-Class Solar Array for NASA's Asteroid Redirect MissionNASA is planning an Asteroid Redirect Mission (ARM) to take place in the 2020s. To enable this multi-year mission, a 40 kW class solar electric propulsion (SEP) system powered by an advanced 50 kW class solar array will be required. Powered by the SEP module (SEPM), the ARM vehicle will travel to a large near-Earth asteroid, descend to its surface, capture a multi-metric ton (t) asteroid boulder, ascend from the surface and return to the Earth-moon system to ultimately place the ARM vehicle and its captured asteroid boulder into a stable distant orbit. During the years that follow, astronauts flying in the Orion multipurpose crew vehicle (MPCV) will dock with the ARM vehicle and conduct extra-vehicular activity (EVA) operations to explore and sample the asteroid boulder. This paper will review the top structural design considerations to successfully implement this 50 kW class solar array that must meet unprecedented performance levels. These considerations include beyond state-of-the-art metrics for specific mass, specific volume, deployed area, deployed solar array wing (SAW) keep in zone (KIZ), deployed strength and deployed frequency. Analytical and design results are presented that support definition of stowed KIZ and launch restraint interface definition. An offset boom is defined to meet the deployed SAW KIZ. The resulting parametric impact of the offset boom length on spacecraft moment of inertias and deployed SAW quasistatic and dynamic load cases are also presented. Load cases include ARM spacecraft thruster plume impingement, asteroid surface operations and Orion docking operations which drive the required SAW deployed strength and damping. The authors conclude that to support NASA's ARM power needs, an advanced SAW is required with mass performance better than 125 W/kg, stowed volume better than 40 kW/cu m, a deployed area of 200 sq m (100 sq m for each of two SAWs), a deployed SAW offset distance of nominally 3-4 m, a deployed SAW quasistatic strength of nominally 0.1 g in any direction, a deployed loading displacement under 2 m, a deployed fundamental frequency above 0.1 Hz and deployed damping of at least 1%. These parameters must be met on top of challenging mission environments and ground testing requirements unique to the ARM project.
Document ID
20160000702
Acquisition Source
Glenn Research Center
Document Type
Conference Paper
Authors
Kerslake, Thomas W.
(NASA Glenn Research Center Cleveland, OH United States)
Kraft, Thomas G.
(NASA Glenn Research Center Cleveland, OH United States)
Yim, John T.
(NASA Glenn Research Center Cleveland, OH United States)
Le, Dzu K.
(NASA Glenn Research Center Cleveland, OH United States)
Date Acquired
January 12, 2016
Publication Date
January 4, 2016
Subject Category
Spacecraft Design, Testing And Performance
Report/Patent Number
GRC-E-DAA-TN26878
Meeting Information
Meeting: AIAA SciTech2016
Location: San Diego, CA
Country: United States
Start Date: January 4, 2016
End Date: January 8, 2016
Sponsors: American Inst. of Aeronautics and Astronautics
Funding Number(s)
WBS: WBS 729200.06.03.02
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Keywords
solar arrays
spacecraft structures
solar electric propulsion
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