title: Experimental shock chemistry of aqueous amino acid solutions and the cometary delivery of prebiotic compounds.
abstract: A series of shock experiments were conducted to assess the feasibility of the delivery of organic compounds to the Earth via cometary impacts. Aqueous solutions containing near-saturation levels of amino acids (lysine, norvaline, aminobutyric acid, proline, and phenylalanine) were sealed inside stainless steel capsules and shocked by ballistic impact with a steel projectile plate accelerated along a 12-m-long gun barrel to velocities of 0.5-1.9 km sec-1. Pressure-temperature-time histories of the shocked fluids were calculated using 1D hydrodynamical simulations. Maximum conditions experienced by the solutions lasted 0.85-2.7 microseconds and ranged from 5.1-21 GPa and 412-870 K. Recovered sample capsules were milled open and liquid was extracted. Samples were analyzed using high performance liquid chromatography (HPLC) and mass spectrometry (MS). In all experiments, a large fraction of the amino acids survived. We observed differences in kinetic behavior and the degree of survivability among the amino acids. Aminobutyric acid appeared to be the least reactive, and phenylalanine appeared to be the most reactive of the amino acids. The impact process resulted in the formation of peptide bonds; new compounds included amino acid dimers and cyclic diketopiperazines. In our experiments, and in certain naturally occurring impacts, pressure has a greater influence than temperature in determining reaction pathways. Our results support the hypothesis that significant concentrations of organic material could survive a natural impact process.
authors: Department of Earth and Planetary Science, University of California, 301 McCone Hall, Berkeley, California 94720-4767, USA.
authors: J G
authors: JG
authors: Blank
authors: G H
authors: GH
authors: Miller
authors: M J
authors: MJ
authors: Ahrens
authors: R E
authors: RE
authors: Winans
mesh_terms: D000596:Amino Acids / Q000737:chemistry*; D018534:Earth, Planet; D019418:Evolution, Chemical; D019419:Evolution, Planetary; D019110:Meteoroids; D000069497:Origin of Life
chemical_list: D000596:Amino Acids