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MOLECULAR-DYNAMICS-NEWS  August 2008

MOLECULAR-DYNAMICS-NEWS August 2008

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Subject:

3rd Titan Chemistry Workshop - First Announcement

From:

arthur suits <[log in to unmask]>

Reply-To:

arthur suits <[log in to unmask]>

Date:

Thu, 21 Aug 2008 13:32:15 -0400

Content-Type:

text/plain

Parts/Attachments:

Parts/Attachments

text/plain (80 lines)

  FIRST ANNOUNCEMENT

Third Workshop on

"Titan Chemistry ; Observations, Experiments, Computations, Modeling"

Caribe Hilton Hotel
San Juan PR Feb 26-28, 2009

http://www.chem.hawaii.edu/Bil301/Titan2009.html

Announcing the third in a series of workshops on the chemistry of 
Titan's atmosphere, co-organized in recent years by Ralf Kaiser, Alex 
Mebel, Ian Sims and Arthur Suits. The meeting will include a mix of 
observation, experiment, theory and modeling, and will include both 
neutral and ion chemistry. We  are planning the workshop to begin with 
registration and a reception  in the evening on Wednesday February 25, 
with Gordon conference style sessions beginning the next morning and 
continuing through mid-day on Saturday the 28th.

Saturn’s moon Titan is the only solar system body besides Earth and 
Venus 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 third in a series of annual meetings aimed to 
better understand the hydrocarbon 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. By focusing on the interplay 
between observational & mission data, modeling, and fundamental 
investigations of the underlying chemical reactions and photochemical 
processes, we also seek emerging generalized concepts on the chemical 
processing of hydrocarbon-rich atmospheres of planets and their moons 
in the Solar System. 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 will feature invited (35 min + 10 min discussion) as well 
as contributed talks (20 min + 5 min discussion) as well as several 
keynote lectures, and is limited to 60 participants. Visits are planned 
to the Arecibo radio observatory as well as El Yunque National Forest.

Further details will be announced in the coming weeks.


Confirmed Speakers:

S. Atreya - Univ. Mich.
J. M. Bowman - Emory Univ.
T. E. Cravens - Univ. Kansas
A. Coustenis - Observtoire Meudon
R. Kaiser - Univ. Hawaii
R. Lorenz - Johns Hopkins
D. Schroeder - IOCB Prague
I. Sims - Univ. Rennes
Mark Smith - Univ. Arizona
A. Suits - Wayne State Univ.
M. Tolbert - Univ. Colorado
V. Vuitton - Grenoble


For further information contact Arthur Suits, [log in to unmask]

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