Condensation in Dust-enriched Systems, by D.S. Ebel and L. Grossman,
Geochimica et Cosmochimica Acta, 1999

Results: Composition of Clinopyroxene

Ca-pxene: 100p3 (thumbnail)

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Figure 11: Composition of spinel as a function of temperature at (a) Ptot= 10-3 bar and a dust enrichment of 100x; (b) Ptot= 10-3 bar and a dust enrichment of 1000x; and (c) Ptot = 10-6 bar and a dust enrichment of 1000x. Inflection points labelled as in Fig. 10, plus: b, perovskite out; c, olivine in; j, liquid out; m, MnO in; n, pyrrhotite in; r, orthopyroxene out.
(enlarge a) (enlarge b) (enlarge c)
Ca-pxene: 1000p3 (thumbnail) The concentrations of FeO, Al2O3 and TiO2 in clinopyroxene are plotted as a function of temperature at 10-3 bar and dust enrichments of 100x and 1000x, and at 10-6 bar and 1000x in Figs. 12a, b and c, respectively. The amount of clinopyroxene increases with falling temperature in all three cases due either to crystallization from the liquid or, after liquid is exhausted, to reactions among plagioclase, orthopyroxene and olivine, as can be seen in Figs. 6 and 7 for the cases at 10-3 bar.
Ca-pxene: 1000p6 (thumbnail) The proportion of the total Fe accounted for by clinopyroxene increases with falling temperature as metal is oxidized, but the concentration of FeO may rise or fall depending on the relative rates of formation of Mg and Fe end-members. Similarly, the proportions of the total Al and Ti accounted for by clinopyroxene increase with falling temperature as this phase crystallizes from the liquid in the cases at 10-3 bar, but the concentrations of Al2O3 and TiO2 may increase or decrease with falling temperature due to the relative formation rates of the different pyroxene end-members. At 10-3 bar and 100x and at 10-6 bar and 1000x, a temperature is reached below which the Al2O3 and TiO2 concentrations begin to fall with decreasing temperature, as plagioclase begins to draw its Al2O3, and pyrophanite its TiO2, from clinopyroxene.




CONDENSATION
in
DUST-ENRICHED SYSTEMS


Denton S. Ebel (1)

Lawrence Grossman(1,2)

(1) Department of The Geophysical Sciences
The University of Chicago
5734 South Ellis Ave.
Chicago, IL 60637

(2) Enrico Fermi Institute
The University of Chicago
5640 South Ellis Ave.
Chicago, IL 60637

Submitted December 22, 1998 to

Geochimica et Cosmochimica Acta

Revised version submitted June 30, 1999
Abstract Introduction
Technique

Bulk Composition
Method of Calculation
Data for Elements and Gas Species
Data and Models for Solids
Data and Models for Silicate Liquids
Test of MELTS: Peridotite KLB-1
Transition Between Liquid Models
Results

Vapor of Solar Composition
General Effects of Dust Enrichment and Total Pressure
Oxygen Fugacity
Condensation Temperatures and Liquid Stability
Condensation at 100x Dust Enrichment, Ptot=10-3bar
Condensation at 1000x Dust Enrichment, Ptot=10-3bar
Condensation of Oxidized Iron at High Temperature
Bulk Chemical Composition of Condensates
Composition of Silicate Liquid
Composition of Spinel
Composition of Clinopyroxene
Composition of Feldspar
Composition of Metallic Nickel-Iron
Metal-Sulfide Condensate Assemblages
Discussion

Stability of Silicate Liquid in Solar Gas
Chondrules in Dust-enriched Systems
Conclusions References