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Also, we outline some evidence for and possible causes of a solar connection in the evolution of atmosphere and climate.
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For details on solar wind influence on the evolution of atmospheres we refer to Lammer et al. (2008) and references therein.
Current analysis suggests that Earth's atmosphere would have evolved to the form found on Venus if the planet had been only 5 percent closer during the evolution of the atmosphere.
Venus remains one of the great unexplored planets in our solar system, with key questions remaining on the evolution of its atmosphere and climate, its volatile cycles, and the thermal and magmatic evolution of its surface.
Finally, the implications of the results for the evolution of the atmospheres of Earth-like planets are discussed.
We present measurements for the production of nitrogen oxides (NO and N2O) in CO2-N2 mixthatsimulateimulate different stages of the evolution of the atmospheres of the Earth, Venus and Mars.
We show that the extreme radiation and plasma environments of the young Sun/stars have important implications for the evolution of planetary atmospheres and may be responsible for the fact that planets with low gravity like early Mars most likely never build up a dense atmosphere during the first few 100 Myr after their origin.
It is shown that the evolution of planetary atmospheres can only be understood if one recognizes the fact that the radiation and particle environment of the Sun or a planet's host star were not always on the same level as at present.
Probably, HCO3- levels had a steady decline due to the reduction of atmospheric CO2, as documented in the evolution of the terrestrial atmosphere [ 31].
The process by which the current atmosphere arose from earlier conditions is complex; however, evidence related to the evolution of Earth's atmosphere, though indirect, is abundant.
The MAVEN mission will explore the evolution of the Martian atmosphere, and will probe whether its cold, thin, dry shell of air was once thick and ideal for microbial life.
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