Venus - Atmospheric evolution.
Thermodynamic equilibrium composition of Venus atmosphere computed from atomic composition deduced spectroscopically
Engineering topics
Publications and source records attributed to Eck, R. V..
Thermodynamic equilibrium composition of Venus atmosphere computed from atomic composition deduced spectroscopically
Thermodynamic equilibrium composition of all combinations of C, H, O and N at average pressure and temperature calculated for atmospheres of earth, Venus, Mars and Jupiter
Jovian atmosphere simulation with energy from corona discharge, producing simple organic molecules
Formation of organic compounds under conditions of thermal equilibrium, noting aromatic compounds in solar nebula and gases activated to plasma state
Thermodynamic equilibrium composition calculations on carbon, hydrogen, oxygen, and nitrogen in Earth, Venus, Mars, and Jupiter atmospheres
Paleogenetic study of ferredoxin structure, reconstructing evolution from amino acid sequence
Thermodynamic equilibria in planetary atmospheres and in origin of organic matter - determination of amino acid pairing and sequences in proteins
Calculation of thermodynamic equilibrium composition of Earth, Venus, Mars and Jupiter atmospheres
Theoretical and experimental support is presented for the hypothesis that organic compounds occurring in carbonaceous chondrites may have formed under equilibrium or near equilibrium conditions. The equilibrium distributions of organic compounds at temperature between 300 and 1000 K and pressures of 10(exp 16) to 50 atmospheres for the C-H-O system have been computed. At high temperatures and low pressures aromatic compounds may form even in the presence of excess hydrogen. Equilibrium concentrations of numerous compounds possible at 1000 K when N, S, and C1 are added to the system have also been determined. A limited equilibrium method is employed in which those few compounds which form with most difficulty are excluded from the computations. This approach is shown to be useful in the interpretation of certain experimental data. In preliminary experiments it has been found that gases, converted to the plasma state by high energy radio frequency discharge, yield product mixtures which are in qualitative agreement with those predicted.
Amino acid sequence of ferredoxin used for determining its evolutionary history
Computer program to compare sequences of amino acids in two proteins to determine regions of identical or related structure
Computer program to formulate matrix of relative deviations from random pairing of amino acids
Expected thermodynamic equilibrium composition calculated for atmospheres of Earth, Venus, Mars, and Jupiter
Complex chemical species and thermodynamic equilibria in prebiological atmospheres