The fate of amino acids during simulated meteoritic impact.

Abstract

Delivery of prebiotic molecules, such as amino acids and peptides, in meteoritic/micrometeoritic materials to early Earth during the first 500 million years is considered to be one of the main processes by which the building blocks of life arrived on Earth. In this context, we present a study in which the effects of impact shock on amino acids and a peptide in artificial meteorites composed of saponite clay were investigated. The samples were subjected to pressures ranging from 12-28.9 GPa, which simulated impact velocities of 2.4-5.8 km/s for typical silicate-silicate impacts on Earth. Volatilization was determined by weight loss measurement, and the amino acid and peptide response was analyzed by gas chromatography-mass spectrometry. For all compounds, degradation increased with peak pressure. At the highest shock pressures, amino acids with an alkyl side chain were more resistant than those with functional side chains. The peptide cleaved into its two primary amino acids. Some chiral amino acids experienced partial racemization during the course of the experiment. Our data indicate that impact shock may act as a selective filter to the delivery of extraterrestrial amino acids via carbonaceous chondrites.

• Authors: Marylène Bertrand, Sjerry van der Gaast, Faith Vilas, Friedrich Hörz, Gerald Haynes, Annie Chabin, Andre Brack, Frances Westall
• Journal: Astrobiology (Astrobiology) Vol. 9 Issue 10 Pg. 943-51 (Dec 2009) ISSN: 1557-8070 [Electronic] United States
• PMID: 20041747 (Publication Type: Journal Article, Research Support, Non-U.S. Gov't)

Chemical References

• Amino Acids
• Dipeptides

Topics

• Amino Acids (analysis, chemistry)
• Dipeptides (analysis, chemistry)
• Gas Chromatography-Mass Spectrometry
• Meteoroids
• Pressure
• Stereoisomerism
• Volatilization