Definition
Titan, Saturn’s moon, is the second largest and only satellite of the solar system having a dense atmosphere composed essentially of dinitrogen (~97%) and methane (~2%). These two molecules give rise to a host of organic compounds, rendering Titan one of the most astrobiologically interesting bodies. In addition, Titan is subject to the effects of seasons and meteorology, shaping the geomorphology of the surface, with unique hydrocarbon liquid bodies and other terrestrial-like features (dunes, channels, mountains). With these properties and the probable existence of an internal liquid water ocean, Titan is a very promising Earth analog which can inform us about the emergence and evolution of life.
Introduction
Astrobiology, the study of life in the universe, is not only the study of the origins, distribution, and evolution of life in the whole universe but also that of structures...
References and Further Reading
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Coustenis, A., Raulin, F. (2019). Titan. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1594-3
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1594-3
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