Hydrocarbon chemistry in the atmosphere of a Warmer Exo-Titan
Hosting a ∼1.5 bar N2 atmosphere and reducing atmospheric composition, Titan has the energy sources needed to drive disequilibrium chemistry and hosts an aerosol layer which shields the surface from incident UV radiation. This world draws parallels to an early Earth-like world (although ∼200 K coole...
| Egile Nagusiak: | , , |
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| Formatua: | Artikulua |
| Hizkuntza: | English |
| Argitaratua: |
Frontiers Media S.A.
2022-09-01
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| Saila: | Frontiers in Astronomy and Space Sciences |
| Gaiak: | |
| Sarrera elektronikoa: | https://www.frontiersin.org/articles/10.3389/fspas.2022.823227/full |