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Titan's organic chemistry : a planetary-scale laboratory to study primitive Earth

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Titan's organic chemistry : a planetary-scale laboratory to study primitive Earth

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dc.contributor.author Coustenis, Athena es
dc.date.accessioned 2021-06-15T08:05:58Z
dc.date.available 2021-06-15T08:05:58Z
dc.date.issued 2016 es
dc.identifier.citation Coustenis, Athena. Titan's organic chemistry : a planetary-scale laboratory to study primitive Earth. En: Mètode Science Studies Journal: Annual Review, 6 2016: 174-181 es
dc.identifier.uri https://hdl.handle.net/10550/79738
dc.description.abstract Saturn?s largest satellite, Titan, has been revealed by extended ground-based and space observations, and recently by the Cassini-Huygens mission. Titan?s atmosphere hosts a complex organic chemistry in the solar system starting with nitrogen and methane and leading to the formation of hydrocarbons and nitriles, including prebiotic molecules. The atmosphere also contains traces of oxygen compounds. This system is subject to seasonal variations and different physical, dynamic, and photochemical processes. Interactions between the atmosphere, the surface, and the interior also play an important role in the astrobiological potential of the satellite. es
dc.title Titan's organic chemistry : a planetary-scale laboratory to study primitive Earth es
dc.type journal article es_ES
dc.subject.unesco es
dc.identifier.doi es
dc.type.hasVersion VoR es_ES

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