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There is now a CONTENT FREEZE for Mercury while we switch to a new platform. It began on Friday, March 10 at 6pm and will end on Wednesday, March 15 at noon. No new content can be created during this time, but all material in the system as of the beginning of the freeze will be migrated to the new platform, including users and groups. Functionally the new site is identical to the old one. webteam@gatech.edu
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Prof. Susanna Widicus Weaver, Emory University
Testing the Limits of Astrochemistry: Integrative Studies in Laboratory Spectroscopy, Observational Astronomy, and Chemical Modeling
Physical Chemistry Divisional Seminar
It is now thought that meteorite and comet impacts delivered water and biological material to the early Earth, seeding the formation of life. Fundamental biological molecules such as amino acids and sugars have been discovered in meteorites, but none of these species have yet been detected in the interstellar medium (ISM). The mechanisms and environments leading to the formation of biologically-relevant molecules therefore remain unclear. While both the number of detected interstellar molecules and their chemical complexity continue to increase, our understanding of the processes leading to their formation is severely lacking. Only interdisciplinary studies with contributions from laboratory spectroscopy, observational astronomy, and chemical modeling will enable us to elucidate the dominant chemical mechanisms in space. In this talk, I will discuss my plans for a research program that fully integrates these three fields of study. In the laboratory, we are developing new high-sensitivity spectral techniques for the terahertz (THz) frequency range. We are combining these techniques with novel production mechanisms to study transient molecules that are key to prebiotic chemical pathways in the ISM. We will use the spectroscopic results as a guide to search for these molecules in space. From these astronomical observations, we can determine the abundance, temperature, and spatial distribution of these species in interstellar clouds. We will then incorporate this information into interstellar chemical models and test the influence of varying physical conditions. The revised models can be used to predict other important chemical pathways, guiding future laboratory and observational studies. Such studies will enable us to pinpoint the interstellar chemical pathways leading to biological molecules and offer clues to the processes leading to the formation of life.
For more information contact Prof. Christine Payne (404-385-3125) or Prof. Thomas Orlando (404-894-4012).
