Evaporation kinetics of forsterite and implications for the early solar nebula

The evaporation kinetics of forsterite, the most abundant mineral in planets and meteorites, were examined.

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Bibliographic Details
Published inNature (London) Vol. 347; no. 6288; pp. 53 - 55
Main Author Hashimoto, Akihiko
Format Journal Article
LanguageEnglish
Published London Nature Publishing 06.09.1990
Nature Publishing Group
Subjects
Astronomy
Astrophysics
Condensation
Crystalline rocks
Earth sciences
Earth, ocean, space
Equilibrium
Equilibrium conditions
Evaporation
Evaporation rate
Exact sciences and technology
Experimental petrology
Experiments
Forsterite
Kinetic energy
Kinetics
Melting point
Melting points
Meteors & meteorites
Mineralogy
Minerals
Oxides
Planets
Rare earth compounds
Reaction kinetics
Silicates
Solar corona
Solar nebula
Solar system
Chondrules
Nesosilicates
Orthosilicates, olivine group
Gaseous phase
Forsterite
Chondrite
Evaporation
Condensation
Silica
Thermodynamics
Experience
Meteorites
Chemical fractionation
Chondrites
Kinetics
Experimental studies
Gas phase
Solar system
Thermodynamic properties
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Summary:The evaporation kinetics of forsterite, the most abundant mineral in planets and meteorites, were examined.
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ISSN:0028-0836
1476-4687
DOI:10.1038/347053a0