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Venus Atmospheric Exploration by Solar AircraftThe Venus atmosphere is a favorable environment for flying powered aircraft. The atmospheric pressure makes flight much easier than on planets such as Mars. Above the clouds, solar energy is available in abundance on Venus, and the slow rotation of Venus allows a solar airplane to be designed for flight within continuous sunlight. The atmosphere between 50 km and 75 km on Venus is one of the most dynamic and interesting regions of the planet. The challenge for a Venus aircraft will be the fierce winds and caustic atmosphere. In order to remain on the sunlit side of Venus, an exploration aircraft will have to be capable of sustained flight at or above the wind speed. An aircraft would be a powerful tool for exploration. By learning how Venus can be so similar to Earth, and yet so different, we will learn to better understand the climate and geological history of the Earth.
Document ID
20030022791
Acquisition Source
Glenn Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Landis, Geoffrey A.
(NASA Glenn Research Center Cleveland, OH, United States)
LaMarre, C.
(Illinois Univ. Champaign, IL, United States)
Colozza, A.
(Analex Engineering Cleveland, OH, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2002
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
IAC-02-Q.4.2.03
Meeting Information
Meeting: 53rd International Astronautical Congress
Location: Houston, TX
Country: United States
Start Date: October 10, 2002
End Date: October 19, 2002
Funding Number(s)
WBS: WBS 22-755-60-02
PROJECT: RTOP 755-A4-02
Distribution Limits
Public
Copyright
Public Use Permitted.
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