Volcanism has been a major process during most of the geologic history of Mars. Based on data collected from terrestrial basaltic eruptions, we assume that the volatile content of martian lavas was typically $0.5 wt.% water, $0.7 wt.% carbon dioxide, $0.14 wt.% sulfur dioxide, and contained several
The potential impact of super-volcanic eruptions on the Earth's atmosphere
β Scribed by Bethan Harris
- Publisher
- John Wiley and Sons
- Year
- 2008
- Tongue
- English
- Weight
- 544 KB
- Volume
- 63
- Category
- Article
- ISSN
- 0043-1656
- DOI
- 10.1002/wea.263
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