Methionine ligand lability of homologous monoheme cytochromes c.

Direct electrochemical analysis of adsorbed bacterial monoheme cytochromes c has revealed a phenomenological loss of the axial methionine when examined using pyrolytic "edge-plane" graphite (EPG) electrodes. While prior findings have reported that the Met-loss state may be quantitatively understood using the cytochrome c from Hydrogenobacter thermophilus as a model system, here we demonstrate that the formation of the Met-loss state upon EPG electrodes can be observed for a range of cytochrome orthologs. Through an electrochemical comparison of the wild-type proteins from organisms of varying growth temperature optima, we establish that Met-ligand losses at graphite surfaces have similar energetics to the "foldons" for known protein folding pathways. Furthermore, a downward shift in reduction potential to approximately -100 mV vs standard hydrogen electrode was observed, similar to that of the alkaline transition found in mitochondrial cytochromes c. Pourbaix diagrams for the Met-loss forms of each cytochrome, considered here in comparison to mutants where the Met-ligand has been substituted to His or Ala, suggest that the nature of the Met-loss state is distinct from either a His-/aquo- or a bis-His-ligated heme center, yet more closely matches the pKa values found for bis-His-ligated hemes., We find the propensity for adoption of the Met-loss state in bacterial monoheme cytochromes c scales with their overall thermal stability, though not with the specific stability of the Fe-Met bond.

Low-energy electron-induced chemistry of condensed methanol: implications for the interstellar synthesis of prebiotic molecules.

In the interstellar medium, UV photolysis of condensed methanol (CH3OH), contained in ice mantles surrounding dust grains, is thought to be the mechanism that drives the formation of "complex" molecules, such as methyl formate (HCOOCH3), dimethyl ether (CH3OCH3), acetic acid (CH3COOH), and glycolaldehyde (HOCH2CHO). The source of this reaction-initiating UV light is assumed to be local because externally sourced UV radiation cannot penetrate the ice-containing dark, dense molecular clouds. Specifically, exceedingly penetrative high-energy cosmic rays generate secondary electrons within the clouds through molecular ionizations. Hydrogen molecules, present within these dense molecular clouds, are excited in collisions with these secondary electrons. It is the UV light, emitted by these electronically excited hydrogen molecules, that is generally thought to photoprocess interstellar icy grain mantles to generate "complex" molecules. In addition to producing UV light, the large numbers of low-energy (< 20 eV) secondary electrons, produced by cosmic rays, can also directly initiate radiolysis reactions in the condensed phase. The goal of our studies is to understand the low-energy, electron-induced processes that occur when high-energy cosmic rays interact with interstellar ices, in which methanol, a precursor of several prebiotic species, is the most abundant organic species. Using post-irradiation temperature-programmed desorption, we have investigated the radiolysis initiated by low-energy (7 eV and 20 eV) electrons in condensed methanol at - 85 K under ultrahigh vacuum (5 x 10(-10) Torr) conditions. We have identified eleven electron-induced methanol radiolysis products, which include many that have been previously identified as being formed by methanol UV photolysis in the interstellar medium. These experimental results suggest that low-energy, electron-induced condensed phase reactions may contribute to the interstellar synthesis of "complex" molecules previously thought to form exclusively via UV photons.