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High pressure equilibria in the iron-nickel system and the structure of metallic meteorites

✍ Scribed by Larry Kaufman; A.E Ringwood


Publisher
Elsevier Science
Year
1961
Weight
622 KB
Volume
9
Category
Article
ISSN
0001-6160

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✦ Synopsis


Calculations of phase eqmlibria in the iron-nickel system at high pressure indicate miscibility gap formation and eutectoid decomposition in iron-nickel alloys at pressures exceeding 60 kb. This behaviour may be the origin of the plessite microstructure, which is an intimate lamellar mixture of low nickel kamacite (b.c.c.) and high nickel taenite (f.c.c.), found in metallic meteorites. EQUILIBRE SOUS HAUTE PRESSION DU SYSTEME FER-NICKEL ET STRUCTURE DES METEORITES METALLIQUES *


πŸ“œ SIMILAR VOLUMES


Density and phase equilibria in the syst
✍ W.B. Streett πŸ“‚ Article πŸ“… 1968 πŸ› Elsevier Science 🌐 English βš– 531 KB

LIQUID-VAPOUR phase data for the system neonnitrogen have been reported in an earlier paper 1 for the temperature range 66.13-120.64Β°K, and at pressures up to 68 atm. These measurements have been extended to higher pressures, and data are reported here at seven temperatures in the range 66.13-114.34