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- W2405917571 abstract "Venus (especially) and Mars have atmospheric compositions strikingly similar to Earth’s near surface volatile inventory. The relative amounts of carbon dioxide and nitrogen, the major gases, not only resemble Earth’s but also resemble the volatile fractions of a putative meteorite mix. The dominance of oxidized gases (even disregarding the oxygen in Earth’s atmosphere) suggest parallels and presumed support for the standard model for terrestrial planet degassing. Detailed consideration of processes that probably affected Venus indicate loss of enormous amounts of hydrogen from its hot atmosphere, to the extent of largely removing it from the planet. The oxygen (from water) left behind is responsible for oxidizing both the surface materials and the reduced carbon compounds that would have been present on early Venus if the current model (highly reduced primordial surface) were applied to Venus." @default.
- W2405917571 created "2016-06-24" @default.
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- W2405917571 date "2015-10-08" @default.
- W2405917571 modified "2023-09-23" @default.
- W2405917571 title "What Can We Learn from Other Planets?" @default.
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- W2405917571 doi "https://doi.org/10.1007/978-3-319-21972-1_12" @default.
- W2405917571 hasPublicationYear "2015" @default.
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