Computer Science
Scientific paper
Jan 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988icar...73..180k&link_type=abstract
Icarus (ISSN 0019-1035), vol. 73, Jan. 1988, p. 180-190.
Computer Science
9
Chemical Composition, Crystal Growth, Iron Compounds, Metal Vapors, Solar Corona, Stellar Composition, Gas Pressure, Interfacial Tension, Interstellar Space
Scientific paper
The homogeneous nucleation and grain growth theory presently applied to the condensation of iron-bearing materials in a gas of solar composition indicates that high supersaturation is needed for iron vapor's homogeneous condensation into metallic form, due to its large surface tension. Such surface-active elements as N, O, S, and P, however, lower the surface tension or iron, and iron atoms can be encapsulated into precondensed MgSiO3 grains as FeO. S is found to be the most effective element in lowering the surface tension of iron in a cooling gas of solar composition.
Hasegawa Hiroichi
Kozasa Takashi
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