Basalt Oxidation and the Formation of Hematite on the Surface of Venus
✍ Scribed by B. Fegley Jr.; G. Klingelhöfer; R.A. Brackett; N. Izenberg; D.T. Kremser; K. Lodders
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 647 KB
- Volume
- 118
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
The reaction of \(\mathrm{N}_{2} \mathrm{O}\) with electrons trapped on the surface of hig gives a complex sienat amsine from the \(\mathrm{O}^{-}\)ion in two or more different sites. The \(0^{-}\)ion reacts with oxyen to give \()_{3}^{-}\)chancierised th strime lines at \(g_{1}=2.0147, g_{2}=2.0120
Thus, the experimental pyrite decomposition rates are relevant to Venus where the S 2 pressure is lower than in the experiments of Fegley et al. The observed sulfur vapor abundance near Venus' surface (1995a). I then consider in situ observations of Venus' lower atmosphere is lower than the amount