A number of experiments simulating the conditions of SHSs were conducted, and abiotic production and polymerization of amino acids were reported. On the other side, it was claimed that organic compounds, particularly amino acids, are not stable AZD6244 in vivo in such high temperature environments as SHSs. In our early studies, not free amino acids but complex amino acids precursors with large molecular weights were formed abiotically from simulated primitive Earth atmosphere (a mixture of CO, N2 and H2O) (Takano et al., 2004). Such complex organics (hereafter referred as to CNW) should have been delivered to SHSs in
primitive ocean, where they were subjected to further alteration. We examined possible alteration of the complex organics in high-temperature high-pressure
environments by the supercritical water flow reactor (SCWFR) (Islam et al. 2003) and an autoclave. The complex amino acid precursors (CNW) were much stabler than free amino acids. While grainy structures of ca. 10 nm size were observed in CNW with a Transmission Electron Microscope (TEM), fused film-like structures of micrometer order size were formed after CNW was heated at 573 K for 2 min by SCWFR. It was possible that complex organic compounds delivered to primordial SHSs altered chemically and morphologically Selleck Tucidinostat toward the generation of the first life. Islam, Md. Tangeritin N., Kaneko, T., and Kobayashi, K (2003). Reactions of Amino Acids with a Newly ConstructedSupercritical Water Flow Reactor Simulating Submarine Hydrothermal Systems. Bull. Chem. Soc. Jpn., 76, 1171 Takano, Y., Marumo, K., Yabashi, S., Kaneko, T., and Kobayashi, K., (2004). Curie-Point
Pyrolysis of Complex Organics Simulated by Cosmic Rays Irradiation of Simple Inorganic Gas Mixture. Appl Pyys. Lett, 85, 1633 E-mail: [email protected]ac.jp Pyrite as a Template for Carbon Fixation Paula Lindgren1, John Parnell2, Nils G. Holm1 1Department of Geology and Geochemistry, Stockholm University, Sweden; 2Department of Geology and Petroleum Geology, University of Aberdeen, UK An important process in the evolution of life is the precipitation and concentration of organic species. There are several examples of minerals acting as templates for the accumulation and concentration of organic matter. These include for instance clays (e.g. Cairns-Smith and Hartman, 1986), radioactive minerals (e.g. Rasmussen, et al. 1993), zeolites and feldspars (e.g. Smith, et al. 1999) and the sulphide mineral pyrite (FeS2) (e.g. Wächtershäuser, 1988). Wächtershäuser (1988) suggested that prebiotic chemistry and eventually life itself could have started on the surface of pyrite.