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Abstract Submission Aldo Apponi
NASA Laboratory Astrophysics Workshop 2006 Abstract Template
Title:
Difficulties in Laboratory Studies and Astronomical Observations of
Organic Molecules: Hydroxyacetone and Lactic Acid
Author(s):
Aldo J. Apponi, James J. Hoy, Matthew Brewster, and Lucy M. Ziurys
The University of Arizona, LAPLACE Astrobiology Center and Steward
Observatory
Abstract:
Organic molecules in interstellar space likely play a role in prebiotic
chemistry. Hence, it is very important to properly identify the
organic species present and to accurately evaluate their abundance.
Owing to the rich molecular spectra found in many interstellar sources,
accurate laboratory rest frequency measurements are crucial to
accomplish these goals.
Two key molecules are hydroxyacetone and lactic acid. A previous study
on hydroxyacetone by Kattija-Ari and Harmony (1980) was not extensive
enough to accurately predict even the A-state of this molecule, which
has a methyl internal rotor. The E-state proved even more difficult as
they found the molecule to possess a very low barrier to internal
rotation. A more recent study by Braakman et al. (2005) provided rest
frequencies for the A-state by measuring its spectrum at 3 mm and 1 mm,
but they too reported that a definitive assignment of the E-state was
proving difficult. Just prior to that time, we started measuring the
microwave spectrum of hydroxyacetone, which was critical for the
assignment of the E-state. We have now extended those measurements to
cover the entire spectrum at 3 and 2 mm, where the strongest low-K
interstellar transitions are predicted. Using the methods described
for fitting low-barrier molecules by Hougan and co-workers and a
modified computer code provided by Kliener et al., we now have fitted
rotational constants that reproduce the data to experimental accuracy
in both the A- and E-states simultaneously. The application of these
methods will be described.
An extensive interstellar search has been conducted for hydroxyacetone
based on these new laboratory results, as well as for lactic acid.
Upper limits to the abundance of these species will be reported along
with a discussion of problems in identifying these and other organic
species owing to a high degree of spectral confusion.
Reference:
Kattija-Ari and Harmony, Inter. J. Quant. Chem., 14, 443 (1980)
Braakman et al., 60th International Symposium on Molecular
Spectroscopy, Columbus, Ohio, Talk RA07