Chemical aspects of the formation of the solar systemApplication of Alfven's theory for the formation of the solar system and the constraints imposed by the chemical composition of space materials are discussed with reference to chemical processes involved in the formation of the solar system. Evidence for the chemical properties of the space medium and the chemical consequences of the postulated physical differentiation processes are outlined, and interpretations based on structure and composition of meteorite material are indicated. A large range of topics, including processes involving chemical differentiation, temperature effects, and isotope fractionation, are examined.
Document ID
19790029033
Acquisition Source
Legacy CDMS
Document Type
Other - Collected Works
Authors
Arrhenius, G. (California, University San Diego, Calif., United States)