The Faint Young Sun Paradox: A Simplified Thermodynamic Approach
Classical models of the Sun suggest that the energy output in the early stage of its evolution was 30 percent less than today. In this context, radiative balance alone between The Sun and the Earth was not sufficient to explain the early presence of liquid water on Earth’s surface. This difficulty i...
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| Autori principali: | , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Wiley
2012-01-01
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| Serie: | Advances in Astronomy |
| Accesso online: | http://dx.doi.org/10.1155/2012/478957 |
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