
TL;DR
Titan's atmosphere and climate are uniquely complex in the solar system, with implications for prebiotic chemistry and habitability, as revealed by Cassini-Huygens data, laboratory work, and models.
Contribution
This review synthesizes current knowledge of Titan's atmosphere and climate, highlighting new insights from recent spacecraft data and laboratory experiments.
Findings
Titan's atmosphere is rich in organic haze and complex chemistry.
Surface-atmosphere interactions shape Titan's dunes and lakes.
Cassini-Huygens data has advanced understanding of Titan's climate system.
Abstract
Titan is the only moon with a substantial atmosphere, the only other thick N atmosphere besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses any other solar system atmosphere, and the only other solar system body with stable liquid currently on its surface. The connection between Titan's surface and atmosphere is also unique in our Solar system; atmospheric chemistry produces materials that are deposited on the surface and subsequently altered by surface-atmosphere interactions such as aeolian and fluvial processes resulting in the formation of extensive dune fields and expansive lakes and seas. Titan's atmosphere is favorable for organic haze formation, which combined with the presence of some oxygen bearing molecules indicates that Titan's atmosphere may produce molecules of prebiotic interest. The combination of organics and liquid, in…
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