Origin of organic matter in early solar system - 1. hydrocarbons.
Identification of hydrocarbons in murray and orgueil meteorites
Engineering topics
Publications and source records attributed to Anders, E..
Identification of hydrocarbons in murray and orgueil meteorites
Ages of calcium-rich achondrites determined by study of 27 eucrites and shergottites
Al 26 content of stony meteorites by coincidence spectrometry noting cosmic ray exposure ages for eight meteorites
Magnetic separations performed on Jodzie howardite, showing uniform primordial gas enrichment indicating covariant solar planetary components
Abundance of volatile elements in meteorites, comparing chondrite decrease for evidence of fractionations in solar nebula
Canyon Diablo meteorite examined, using mass spectrometry and metallography, noting shock effects
Critique of paper by Carter and Kennedy regarding origin of diamonds in Canyon Diablo and Novo Urei meteorite
Formation of hydrocarbons by Fischer-Tropsch reaction involving carbon monoxide, hydrogen, and meteorites
Aromatic hydrocarbons in carbonaceous chondrites investigated by time-of-flight mass spectrometry and hypothesized as formed in solar nebula under thermodynamic equilibrium
Chemical fractionations in meteorites - acceptance of chondrites as average samples of nonvolatile planetary matter
Fragmentation history of asteroids derived from absolute magnitude distribution resembling Gaussian curve for brighter members and logarithmic curve for fainter ones
S-34 to S-32 ratio for elemental, troilite and sulfate sulfur in Orgueil meteorite and mode of formation
Meteorite of Orgueil shower showing contamination examined as hoax
Meteorite contaminated with biogenic materials - plant fragments, hydrocarbons, and water soluble proteins
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