Titan (Satellite) Atmosphere

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Information for Authority record

Name (Hebrew)
טיטן (לווין) אטמוספרה
Name (Latin)
Titan (Satellite) Atmosphere
Other forms of name
Atmosphere of Titan
Titanian atmosphere
MARC
MARC

Other Identifiers

Wikidata: Q1143812
Library of congress: sh2005020197
Sources of Information
  • Work cat.: Bouchez, A.H. Seasonal trends in Titan's atmosphere, 2004.
  • 74601355: The atmosphere of Titan, 1974.
  • Sagan, C. "No small rapture" : the exploration of Saturn's extraordinary moon, Titan, via WWW, Mar. 31, 2005(Titanian atmosphere; atmosphere of Titan)
  • The Titanian paradox, via Titan exploration web site, Mar. 31, 2005(Titan's atmosphere; Titanian atmosphere)
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Wikipedia description:

The atmosphere of Titan is the dense layer of gases surrounding Titan, the largest moon of Saturn. Titan is the only natural satellite of a planet in the Solar System with an atmosphere that is denser than the atmosphere of Earth and is one of two moons with an atmosphere significant enough to drive weather (the other being the atmosphere of Triton). Titan's lower atmosphere is primarily composed of nitrogen (94.2%), methane (5.65%), and hydrogen (0.099%). There are trace amounts of other hydrocarbons, such as ethane, diacetylene, methylacetylene, acetylene, propane, PAHs and of other gases, such as cyanoacetylene, hydrogen cyanide, carbon dioxide, carbon monoxide, cyanogen, acetonitrile, argon and helium. The isotopic study of nitrogen isotopes ratio also suggests acetonitrile may be present in quantities exceeding hydrogen cyanide and cyanoacetylene. The surface pressure is about 50% higher than on Earth at 1.5 bars (147 kPa). This is higher than the pressure at the triple point of methane, which allows there to be liquid methane on the surface in addition to the gaseous methane in the atmosphere. The orange color as seen from space is produced by other more complex chemicals in small quantities, possibly tholins, tar-like organic precipitates.

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