Organic geochemical studies. I.
Organic geochemical criteria for differentiating molecules originating from biological and nonbiological processes, noting isoprenoid hydrocarbons genesis problems
Engineering topics
Publications and source records attributed to Calvin, M..
Organic geochemical criteria for differentiating molecules originating from biological and nonbiological processes, noting isoprenoid hydrocarbons genesis problems
Chemical evolution and geologic history of earth, and molecular structures of organic compounds
Oils and shales from 3 million to 2.7 billion years old analyzed for hydrocarbon content, using gas chromatography and mass spectrometry
Planetary reflection spectroscopy for studying extraterrestrial life
Column chromatography used to determine hydrocarbons present in Moonie crude oil from Queensland, Australia, that is two hundred million years old
Chemical analysis of sediment and oil hydrocarbon content by gas chromatography and mass spectrometry to establish inception period of bio-organic evolution
Adenine synthesis by electron irradiation of gas mixture of methane, ammonia, and water
Isolation and identification of biogenic steranes and pentacyclic triterpanes in Eocene shale
Possible biological origin of isoprenoid alkanes found in sediments 30 million and 2-1/2 billion years old
Evidence of life processes in sediment over two billion years old as related to biological or abiological origin of hydrocarbons from meteorites
Isolation of isoprenoid hydrocarbons from alkane fractions in Precambrian sediment and associated oil seepage
Occurrence of biogenic steranes and cyclic triterpanes in very old, carbonaceous sediment rock formations - Green River shale, and Soudan shale fragmentation components
Discussion on reflection spectra of bioorganic materials and its use in evaluating absorption bands of mars
Interpretation of the 3-to 4- micron spectrum of mars through the study of infrared reflection spectra of organic and inorganic materials
Infrared reflection spectra have been recorded for a large number of inorganic and organic samples, including minerals and biological specimens, for the purpose of interpreting the 3- to 4-micron spectrum of Mars. A previous suggestion that the Martian bands indicated the presence of carbohydrates is shown not to be a required conclusion. However, no satisfactory explanation is advanced and the problem remains unresolved.
Reflection spectra of bio-organic materials and its use in evaluating the absorption bands of mars