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Prebiotic Molecules in the Interstellar Medium Susanna L. Widicus Weaver Department of Chemistry Emory University. H. He. Ne. O. C. N. Si. S. Ar. Mg. Fe. The Astronomer’s Periodic Table. Detected Interstellar Molecules. Schematic of a Hot Core. T (gas) = 200 - 1000 K.
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Prebiotic Molecules in the Interstellar Medium Susanna L. Widicus Weaver Department of Chemistry Emory University
H He Ne O C N Si S Ar Mg Fe The Astronomer’s Periodic Table Detected Interstellar Molecules
Schematic of a Hot Core T (gas) = 200 - 1000 K T (dust) ~90 K ~60 K ~45 K ~20 K CO2 CO N2 O2 ice complex organics H2O, CH3OH, NH3 H2S CH3OH ice SiO CH3CN CO2 ice trapped CO UV H2O ice Hot Core ~1016 cm ~5x1017 cm
Organic Material in Meteorites • The Murchison Meteorite • amino acids • sugars and polyols • other organics
Possible Molecular Formation Schemes vs. Key Questions: How far can chemistry go in the ISM?? Is a parent body required??
Laboratory Modeling Molecules of Interest Reaction Kinetics & Dynamics, Molecular Parameters Unidentified Lines Abundance Predictions Observations Physical Conditions, Molecular Abundances Transition Frequencies & Strengths Prebiotic Astrochemistry Research