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6533b830fe1ef96bd12970f3

RESEARCH PRODUCT

Methane in Titan's atmosphere: from fundamental spectroscopy to planetology

Vincent BoudonCaitlin A. GriffithEmmanuel LellouchAlberto NegrãoAlberto NegrãoPierre DrossartMathieu HirtzigTony GabardBruno BézardCatherine De BerghMichel LoeteJean Paul ChampionAthena Coustenis

subject

Origin of water on EarthGeneral Physics and AstronomyMethane[PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Astrobiologychemistry.chemical_compoundsymbols.namesakeNatural gasPlanetologiePhysics::Chemical PhysicsAtmosphere of TitanAstrophysics::Galaxy AstrophysicsPhysics::Atmospheric and Oceanic PhysicsSpectroscopyLife on Titanbusiness.industryPlanetary sciencechemistryGreenhouse gasPhysics::Space PhysicssymbolsEnvironmental scienceAstrophysics::Earth and Planetary AstrophysicsbusinessTitan (rocket family)Titan[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Methane

description

The methane molecule (CH4) is relatively abundant in the Universe and in particular in our Solar System. On Earth, it is the main compound of natural gas and is also the second greenhouse gas of anthropic origin. On Saturn's satellite Titan it plays a role similar to water on Earth and leads to a complex chemistry.

yearjournalcountryeditionlanguage
2009-07-01
10.1051/epn/2009601https://hal.science/hal-03724249/file/epn20094p16.pdf
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