P31C:
Titan: Constraining an Ocean World I Posters
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P31C:
Titan: Constraining an Ocean World I Posters
Titan: Constraining an Ocean World I Posters
You can still search the program to see your colleague�s abstract submissions as well as the sessions submitted for the 2016 Fall Meeting. The final program will be released in early October.
Session ID#: 12714
Session Description:
The joint NASA/ESA Cassini mission has established Titan as a prime location for investigating the limits of life. Cassini has studied Titan’s interior, seasonal changes on its surface and atmosphere, and the atmosphere’s interaction with an energetic magnetosphere. Cassini finds surface-atmosphere interactions producing erosional features similar to Earth’s, including dunes, mountains, rivers, alluvial deposits, and features suggesting recent cryovolcanism. There is also evidence for a salty ocean interior and accumulations of liquid hydrocarbons are evident on its surface. The atmosphere’s interaction with the magnetosphere produces a continuous supply of new organic material. The inclusion of Titan as a target for exploration by missions under NASA’s New Frontiers program highlights broad solar system community interest in this scientifically rich moon. This session will explore new results that intend to provide a comprehensive and integrated understanding of Titan’s interior, surface, and atmosphere, along with the atmosphere’s interaction with the Saturn’s energetic environment.
Primary Convener: Robert M. Nelson, Planetary Science Institute Tucson, Tucson, AZ, United States
Conveners: Conor A Nixon, NASA Goddard Space Flight Center, Planetary Systems Laboratory, Greenbelt, MD, United States, Joe H Westlake, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
Chairs: Conor A Nixon, NASA Goddard Space Flight Center, Planetary Systems Laboratory, Greenbelt, MD, United States, Joe H Westlake, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Robert M. Nelson, Planetary Science Institute Tucson, Tucson, AZ, United States and Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
OSPA Liaison: Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
Index Terms:
5405 Atmospheres [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
5443 Magnetospheres [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
6280 Saturnian satellites [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6281 Titan [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
Abstracts Submitted to this Session:
The Role of 1CH2 Chemistry in Determining Ethane and Benzene Formation in Titan's Atmosphere (149527)
Titan's gravity: An update (152219)
See more of: Planetary Sciences
