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Progress of the Dust Accumulation and Removal Technology Experiment (DART) for the Mars 2001 LanderDust deposition could be a significant problem for photovoltaic array operation for long duration missions on the surface of Mars. Measurements made by Pathfinder showed 0.3 percent loss of solar array performance per day due to dust obscuration. We have designed an experiment package, "DART", which is part of the Mars ISPP Precursor (MIP) package, to fly on the Mars-2001 Surveyor Lander. This mission, to launch in April 2001, will arrive on Mars in January 2002. The DART experiment is designed to quantify dust deposition from the Mars atmosphere, measure the properties of settled dust, measure the effect of dust deposition on array performance, and test several methods of clearing dust from solar cells.
Document ID
20050203759
Acquisition Source
Glenn Research Center
Document Type
Conference Paper
Authors
Jenkins, Phillip
(NASA Glenn Research Center Cleveland, OH, United States)
Landis, Geoffrey A.
(NASA Glenn Research Center Cleveland, OH, United States)
Wilt, David
(NASA Glenn Research Center Cleveland, OH, United States)
Krasowski, Michael
(NASA Glenn Research Center Cleveland, OH, United States)
Greer, Lawrence
(NASA Glenn Research Center Cleveland, OH, United States)
Baraona, Cosmo
(NASA Glenn Research Center Cleveland, OH, United States)
Scheiman, David
(NASA Glenn Research Center Cleveland, OH, United States)
Date Acquired
September 7, 2013
Publication Date
May 1, 2005
Publication Information
Publication: 16th Space Photovoltaic Research and Technology Conference
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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