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Proposal for a Sample Return from TitanWe propose to explore a Titan sample return mission using in-situ volatile propellants available on its surface. Titan is unique in the outer solar system in that it is the only moon with a thick atmosphere, andthe only body in the solar system outside the Earth with liquid seas on its surface. The Titanian oceans, however, are seas of liquid hydrocarbons, and the rocks on the surface are solid water ice. Many studies of space development emphasize use of the in-situ resources to eliminate the requirement to launch propellants from Earth. With water, liquid methane,and ethane easily available, Titan is a rocket scientist’s dream for propellants.
Document ID
20210017381
Acquisition Source
Glenn Research Center
Document Type
Presentation
Authors
Geoffrey A Landis
(Glenn Research Center Cleveland, Ohio, United States)
Steven R Oleson
(Glenn Research Center Cleveland, Ohio, United States)
Date Acquired
June 11, 2021
Subject Category
Spacecraft Propulsion And Power
Meeting Information
Meeting: 18th Planetary Probe Workshop
Location: Virtual
Country: US
Start Date: June 17, 2021
End Date: August 17, 2021
Sponsors: Analytical Mechanics Associates (United States)
Funding Number(s)
WBS: 371544.01.21.01.22.01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Technical Review
Single Expert
Keywords
Titan
Propellants
Titan Launch Vehicle
Power
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