OXIDATION OF LOW-CARBON STEEL IN MULTICOMPONENT GASES .1. REACTION-MECHANISMS DURING ISOTHERMAL OXIDATION

Citation
Ht. Abuluwefa et al., OXIDATION OF LOW-CARBON STEEL IN MULTICOMPONENT GASES .1. REACTION-MECHANISMS DURING ISOTHERMAL OXIDATION, Metallurgical and materials transactions. A, Physical metallurgy andmaterials science, 28(8), 1997, pp. 1633-1641
Citations number
14
Categorie Soggetti
Metallurgy & Metallurigical Engineering","Material Science
ISSN journal
10735623
Volume
28
Issue
8
Year of publication
1997
Pages
1633 - 1641
Database
ISI
SICI code
1073-5623(1997)28:8<1633:OOLSIM>2.0.ZU;2-7
Abstract
The article describes rates of oxidation of low carbon steel in variou s nitrogen-based atmospheres of O-2, CO2, and H2O in the temperature r ange 800 degrees C to 1150 degrees C. In characterizing the oxidation process, the weight gains of the samples per unit surface area vs time data were analyzed. Reaction rates during oxidation in the binary atm ospheres of CO2-N-2 and H2O-N-2 followed a linear rate law and were fo und to be proportional to the partial pressures of CO2 or H2O. These r ates were controlled by rate of reactions at the oxide surface and wer e highly dependent on oxidation temperature. The activation energies o f the phase boundary reactions obtained were approximately 274 and 264 kJ/mole, for oxidation in CO2 and H2O atmospheres, respectively. Oxid ation in gases containing free oxygen showed that the main oxidizing a gent was the free oxygen and that additions of CO2 and H2O had little effect on the magnitude of the initial oxidation rates. Experiments fo r oxidation in multicomponent gases showed that the overall oxidation rates were the additions of rates resulting from oxidation with the in dividual gaseous species O-2, CO2, and H2O. Oxidation in these atmosph eres exhibited an initial linear rate law which gradually transformed into a parabolic. Examination of scale microstructure after 1 hour of oxidation showed that, for oxidation in carbon dioxide and water vapor atmospheres, only wustite was present, while in atmospheres containin g free oxygen, all three iron oxides, wustite, magnetite, and hematite , were present.