Abstract

The condensation temperatures of refractory silicates and oxides in a gas of cosmic composition are strongly dependent on the C O ratio. As the ratio increases from 0.4 to 0.9 (solar ~ cosmic ~ 0.6), condensation temperatures of compounds such as A1 2O 3, Ca 2Al 2SiO 7, MgAl 2O 4, Mg 2SiO 4 and MgSiO 3 decrease by 50–100°. As C O increases from 0.9 to 1.0, these temperatures drop an additional 300–400°. Other chemical differences result when C O $ ̆ 0.9 include: a new suite of high temperature minerals appears (graphite, CaS, Fe 3C, SiC and TiN); the reaction CO + 3H 2 → CH 4 + H 2O proceeds to the right at higher temperatures; and iron, whose condensation temperature is unaffected, condenses at higher temperatures than any silicate or oxide.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.