Compact Telescoping Surface Array for Mars Solar Power
Author(s) -
Richard S. Pappa,
G. Rose,
Matthew K. Chamberlain,
Dave Paddock,
Martin M. Mikulas
Publication year - 2018
Publication title -
nasa sti repository (national aeronautics and space administration)
Language(s) - English
Resource type - Conference proceedings
DOI - 10.2514/6.2018-1944
Subject(s) - telescoping series , mars exploration program , astrobiology , surface (topology) , power (physics) , electrical engineering , computer science , materials science , physics , engineering , mechanical engineering , mathematics , geometry , quantum mechanics
This paper describes a lightweight, large-area solar array concept for Mars surface power called the Compact Telescoping Surface Array (CTSA). The design is derived from the Compact Telescoping Array (CTA) proposed in 2015 for high-power spacecraft. The CTSA deploys horizontally from Mars landers, provides 1000 m of solar cell area, and generates about 50-80 kW daytime and 10 kW nighttime power (from energy storage) near the equator with clear skies. The total mass is about 1500 kg, and the stowed volume is about 10 m, equivalent to 200 W/kg and 30 kW/m at 1 astronomical unit (AU) from the sun. These challenging mass and volume goals require compact, lightweight structures to deploy and tension thin solar cell blankets in the Mars 0.38 g gravity field. Other features include singleaxis rotation for daily or seasonal sun tracking, dust shedding, and feathering in high winds and sufficient strength for sustained 40 m/s winds in dust storms and brief 100 m/s winds in dust devils (dynamic pressure of 120 Pa). Based on preliminary design and analysis reported in the paper, CTSA appears to be a feasible approach for 1000 m-class Mars solar arrays that autonomously deploy from landers prior to human arrival.
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