Journal Article10.1016/J.PSS.2006.05.028
Titan's methane cycle
Sushil K. Atreya,E. Y. Adams,Hasso B. Niemann,Jaime E. Demick-Montelara,Tobias Owen,Marcello Fulchignoni,Francesca Ferri,Eric Wilson +7 more
TL;DR: In this paper, a complex photochemical-meteorological-hydrogeochemical cycle of methane operates on Titan and it is shown that although photochemistry leads to the loss of methane from the atmosphere, conversion to a global ocean of ethane is unlikely.
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About: This article is published in Planetary and Space Science. The article was published on 01 Oct 2006. The article focuses on the topics: Life on Titan & Atmosphere of Titan.
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Citations
Composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini‐Huygens probe gas chromatograph mass spectrometer experiment
Hasso B. Niemann,S. K. Atreya,J. E. Demick,D. Gautier,J. A. Haberman,D. N. Harpold,Wayne Kasprzak,Jonathan I. Lunine,Tobias Owen,François Raulin +9 more
TL;DR: The Cassini-Huygens Probe Gas Chromatograph Mass Spectrometer (GCMS) determined the composition of the Titan atmosphere from ~140km altitude to the surface as mentioned in this paper.
•Book
Atmospheric Evolution on Inhabited and Lifeless Worlds
David C. Catling,James F. Kasting +1 more
- 10 May 2017
TL;DR: In this article, the authors present a survey of the current understanding of the atmospheric evolution and climate on Earth, on other rocky planets within our Solar System, and on planets far beyond.
397
Photochemistry in Terrestrial Exoplanet Atmospheres I: Photochemistry Model and Benchmark Cases
TL;DR: In this paper, a comprehensive photochemistry model for exploration of the chemical composition of terrestrial exoplanet atmospheres is presented, which treats up to 800 chemical reactions, photochemical processes, dry and wet deposition, surface emission, and thermal escape of O, H, C, N, and S bearing species, as well as formation and deposition of elemental sulfur and sulfuric acid aerosols.
337
Temperatures of aqueous alteration and evidence for methane generation on the parent bodies of the CM chondrites
Weifu Guo,John M. Eiler +1 more
TL;DR: Aqueous alteration of primitive meteorites was among the earliest geological processes during the evolution of our solar system as mentioned in this paper, leading to the occurrence of methane on Titan, Triton, Pluto, and other Kuiper-belt objects.
243
Titan's atmosphere and climate
TL;DR: Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses any other solar system atmosphere, and the only solar system body with stable liquid currently on its surface as mentioned in this paper.
236
References
A Serpentinite-Hosted Ecosystem: The Lost City Hydrothermal Field
Deborah S. Kelley,Jeffrey A. Karson,Gretchen L. Früh-Green,Dana R. Yoerger,Timothy M. Shank,David A. Butterfield,John M. Hayes,Matthew O. Schrenk,Eric J. Olson,Giora Proskurowski,Michael V. Jakuba,A. M. Bradley,Ben Larson,Kristin A. Ludwig,Deborah Glickson,Kate Buckman,Alexander S. Bradley,William J. Brazelton,Kevin K. Roe,Mitch J. Elend,Adélie Delacour,Stefano M. Bernasconi,Marvin D. Lilley,John A. Baross,Roger E. Summons,Sean P. Sylva +25 more
TL;DR: The serpentinite-hosted Lost City hydrothermal field is a remarkable submarine ecosystem in which geological, chemical, and biological processes are intimately interlinked.
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Photochemistry of the atmosphere of Titan: comparison between model and observations.
TL;DR: The photochemistry of simple molecules containing carbon, hydrogen, nitrogen, and oxygen atoms in the atmosphere of Titan has been investigated using updated chemical schemes and the authors' own estimates of a number of key rate coefficients, which satisfactorily accounts for the concentrations of minor species observed by the Voyager IRIS and UVS instruments.
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The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe
Hasso B. Niemann,Sushil K. Atreya,Siegfried Bauer,G. R. Carignan,J. E. Demick,R. L. Frost,D. Gautier,J. A. Haberman,D. N. Harpold,Donald M. Hunten,G. Israel,Jonathan I. Lunine,Wayne Kasprzak,Tobias Owen,Michael B. Paulkovich,François Raulin,E. Raaen,S. Way +17 more
TL;DR: Direct atmospheric measurements from the Gas Chromatograph Mass Spectrometer (GCMS), including altitude profiles of the constituents, isotopic ratios and trace species (including organic compounds), were reported, confirming the primary constituents were confirmed to be nitrogen and methane.
Detection of Methane in the Atmosphere of Mars
Vittorio Formisano,Sushil K. Atreya,Thérèse Encrenaz,Nikolai Ignatiev,Nikolai Ignatiev,Marco Giuranna +5 more
TL;DR: A detection of methane in the martian atmosphere by the Planetary Fourier Spectrometer onboard the Mars Express spacecraft is reported, and the global average methane mixing ratio is found to be 10 ± 5 parts per billion by volume.
Rain, winds and haze during the Huygens probe's descent to Titan's surface
Martin G. Tomasko,Brent A. Archinal,Tammy L. Becker,Bruno Bézard,M. Bushroe,M. Combes,D. Cook,Athena Coustenis,C. de Bergh,L. E. Dafoe,Lyn R. Doose,Sylvain Douté,A. Eibl,S. Engel,Fritz Gliem,B. Grieger,K. Holso,Elpitha Howington-Kraus,Erich Karkoschka,H. U. Keller,Randolph L. Kirk,R. Kramm,Michael Küppers,Peter Lanagan,E. Lellouch,Mark T. Lemmon,Jonathan I. Lunine,Jonathan I. Lunine,Elisabeth A. McFarlane,John E. Moores,G. M. Prout,Bashar Rizk,Mark R. Rosiek,P. Rueffer,Stefan Schröder,Bernard Schmitt,C. See,Paul S. Smith,Laurence A. Soderblom,Nicolas Thomas,Robert West +40 more
TL;DR: Spectra and high-resolution images obtained by the Huygens Probe Descent Imager/Spectral Radiometer instrument in Titan's atmosphere reveal the traces of once flowing liquid, and like Earth, the brighter highland regions show complex systems draining into flat, dark lowlands.
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