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First Workshop on Titan - Observations, Experiments, Computations, and Modeling
Honolulu, Hawaii, February 5-7, 2007
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Saturn's moon Titan is the only solar system body besides Earth with a
thick atmosphere and is widely considered as a natural laboratory on
the planetary scale to understand the prebiotic chemistry on
proto-Earth. The Cassini-Huygens mission to Titan has opened a new
chapter in Solar System exploration and extraterrestrial atmospheric
chemistry. On January 14, 2005, the Huygens probe successfully
descended through the atmosphere of Titan and safely landed on its
surface. An extraordinary new world has been unveiled. The scientific
data obtained by the Huygens experiments and by the Cassini Orbiter -
currently being archived and analyzed are far from being understood.
This workshop is part of the NSF-Collaborative Research in Chemistry
(CRC) Network "Chemistry of Unsaturated Hydrocarbons in Titan's
Atmosphere and the first in a series of annual meetings aimed to better
understand the chemistry taking place in the atmosphere and on the
surface of Titan. It brings together atmospheric modelers, astronomical
observers, mission specialists, planetary scientists, physical chemists
(dynamics, kinetics, photochemistry), theoreticians (electronic
structure, dynamics calculations), astrobiologists, and organic
chemists (hydrocarbon and nitrile chemistry). By exploring the current
boundaries of planetary science and chemical knowledge, we can more
effectively design new laboratory experiments under well-defined
conditions (and recommend promising directions for further
observational searches) and upcoming Solar System missions to resolve
hitherto unanswered aspects of molecular synthesis in our Solar
System.
The workshop features invited (40 min + 10 min discussion) as well as
contributed talks (15 min + 5 min discussion) and is limited to 50
participants. A special session is dedicated to needs for laboratory,
computational, modeling, and observational data. Registration forms
and abstracts shall be submitted as outlined in the attachments
(deadline: December 31, 2006). Abstract are only accepted in electronic
form (doc/pdf; titan@gold.chem.hawaii.edu Additional information on
speakers, the conference venue, and accommodations will be added on the
web site as they become available
(http://www.chem.hawaii.edu/Bil301/Titan2007.html). For additional
questions, please email to titan@gold.chem.hawaii.edu.
We are looking forward to seeing you in Honolulu. |
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