Titan's Atmosphere and Climate

@inproceedings{Horst2017TitansAA,
  title={Titan's Atmosphere and Climate},
  author={S. Horst},
  year={2017}
}
Titan is the only moon with a substantial atmosphere, the only other thick N$_{2}$ 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… Expand
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The floatability of aerosols and wave damping on Titan’s seas
Titan, the enigmatic large moon of Saturn, is unique because it is the only satellite of the solar system that is surrounded by a dense atmosphere. Thick layers of photochemical organic aerosols… Expand
A post-Cassini view of Titan’s methane-based hydrologic cycle
The methane-based hydrologic cycle on Saturn’s largest moon, Titan, is an extreme analogue to Earth’s water cycle. Titan is the only planetary body in the Solar System, other than Earth, that is… Expand
Study of Titan’s Upper and Lower Atmosphere : An Experimental Approach
Titan is the only moon in the SolarSystem to possess its own dense and gravitationallybound atmosphere, and is even larger than planetMercury. Its rocky diameter is a mere 117 km shy ofGanymede’s. If… Expand
Dune Formation and Sand Transportation on Titan
Nearly 20% of Titan’s surface is covered with equatorial linear dunes similar to sand dunes on Earth. However, the sand on Titan is not made of silicates, as on Earth, but mainly of organic materials… Expand
The evolution of Titan’s high-altitude aerosols under ultraviolet irradiation
The Cassini–Huygens space mission revealed that Titan’s thick brownish haze is initiated high in the atmosphere at an altitude of about 1,000 km, before a slow transportation down to the surface.… Expand
Low-temperature synthesis of polycyclic aromatic hydrocarbons in Titan’s surface ices and on airless bodies
TLDR
It is revealed in laboratory simulation experiments that aromatics such as benzene, naphthalene, and phenanthrene—prospective building blocks of the organic dune material—can be efficiently synthesized via galactic cosmic ray exposure of low-temperature acetylene ices on Titan's surface, hence challenging conventional wisdom that aromatic hydrocarbons are formed solely in Titan’s atmosphere. Expand
Laboratory investigations of Titan haze formation: In situ measurement of gas and particle composition
Abstract Prior to the arrival of the Cassini-Huygens spacecraft, aerosol production in Titan’s atmosphere was believed to begin in the stratosphere where chemical processes are predominantly… Expand
Energy Delivery via Meteors into Titan's Atmosphere
The Cassini-Huygens mission measured the chemical abundances of the major components of Titan’s atmosphere, and analyses of the data revealed several as-yet unexplained anomalies in themethane and… Expand
Possible explosion crater origin of small lake basins with raised rims on Titan
The Cassini mission discovered lakes and seas comprising mostly methane in the polar regions of Titan. Lakes of liquid nitrogen may have existed during the epochs of Titan’s past in which methane was… Expand
Cryovolcanism and Degassing on Titan, a Moon of Saturn
Abstract— This paper considers the occurrence, diversity, and special features of volcanic and degassing processes on Titan, as well as analyzing the maximum gas concentrations of volatiles in a… Expand
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