DocumentCode :
1484995
Title :
Lunar and Martian Dust Dynamics
Author :
Mazumder, M.K. ; Srirama, P.K. ; Sharma, R. ; Biris, A.S. ; Hidetaka, I. ; Trigwell, S. ; Horenstein, M.N.
Author_Institution :
Boston Univ., Boston, MA, USA
Volume :
16
Issue :
4
fYear :
2010
Firstpage :
14
Lastpage :
21
Abstract :
In order to support human and robotic explorations of Mars and beyond,the National Aeronautics and Space Administration (NASA) has undertaken lunar missions. One technological problem is the mitigation of dust hazards associated with both lunar and Mars missions. There are many factors that transformed lunar regolith into an ocean dust like volcanic eruption, meteorite impact, solar radiation and thermal cycling, solar plasma and bombardment by interplanetary dusts. A detailed understanding of lunar and Martian dust dynamics is needed for designing and implementing dust hazard mitigation methods to facilitate successful missions to the moon and Mars.
Keywords :
Mars; aerospace robotics; cosmic dust; lunar surface; planetary volcanism; solar radiation; Mars; Martian dust dynamics; National Aeronautics and Space Administration; interplanetary dusts; lunar missions; lunar regolith; meteorite impact; robotic explorations; solar plasma; solar radiation; volcanic eruption;
fLanguage :
English
Journal_Title :
Industry Applications Magazine, IEEE
Publisher :
ieee
ISSN :
1077-2618
Type :
jour
DOI :
10.1109/MIAS.2010.936969
Filename :
5458477
Link To Document :
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