P031
Tangerine Dream: Titan’s Diverse Environments
Tangerine Dream: Titan’s Diverse Environments
Session ID#: 162209
Session Description:
Titan is the only moon in the Solar System with a dense atmosphere. It is an Ocean World, with an interior liquid water layer that may provide an abode for life. Photochemistry in the stratosphere consumes methane and generates complex organic molecules, perhaps analogous to the atmospheric chemistry of prebiotic Earth, and in the present-day atmospheres of exoplanets. Methane meteorology in the lower atmosphere leads to rivers, seas, clouds and rain in a weather cycle analogous to that on Earth. The surface has few craters, but exhibits mountains, dune fields and other mysterious landforms that may be evidence for ongoing tectonism. Titan has been highlighted as an important destination for future exploration in the 2022 Decadal Survey for Planetary Sciences, including NASA’s Dragonfly mission, and a possible future Titan Orbiter. In this session we welcome new research relevant to Titan, including observations, spacecraft data analysis, modeling and laboratory experiment work. We also welcome abstracts that discuss relevance of Titan observations to exoplanet studies.
Index Terms:
5210 Planetary atmospheres, clouds, and hazes [PLANETARY SCIENCES: ASTROBIOLOGY]
5225 Early environment of Earth [PLANETARY SCIENCES: ASTROBIOLOGY]
6207 Comparative planetology [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6281 Titan [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
Primary Convener: Conor A Nixon, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Conveners: Alexander Hayes, Cornell University, Department of Astronomy, Ithaca, United States, Kathleen Mandt, The Johns Hopkins University Applied Physics Laboratory, Space Exploration Sector, Laurel, MD, United States and Christophe Sotin, Jet Propulsion Laboratory-California Institute of Technology, Pasadena, CA, United States
See more of: Planetary Sciences
