Literature DB >> 17495166

The process of tholin formation in Titan's upper atmosphere.

J H Waite1, D T Young, T E Cravens, A J Coates, F J Crary, B Magee, J Westlake.   

Abstract

Titan's lower atmosphere has long been known to harbor organic aerosols (tholins) presumed to have been formed from simple molecules, such as methane and nitrogen (CH4 and N2). Up to now, it has been assumed that tholins were formed at altitudes of several hundred kilometers by processes as yet unobserved. Using measurements from a combination of mass/charge and energy/charge spectrometers on the Cassini spacecraft, we have obtained evidence for tholin formation at high altitudes (approximately 1000 kilometers) in Titan's atmosphere. The observed chemical mix strongly implies a series of chemical reactions and physical processes that lead from simple molecules (CH4 and N2) to larger, more complex molecules (80 to 350 daltons) to negatively charged massive molecules (approximately 8000 daltons), which we identify as tholins. That the process involves massive negatively charged molecules and aerosols is completely unexpected.

Entities:  

Mesh:

Substances:

Year:  2007        PMID: 17495166     DOI: 10.1126/science.1139727

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  27 in total

1.  Organic Haze as a Biosignature in Anoxic Earth-like Atmospheres.

Authors:  Giada Arney; Shawn D Domagal-Goldman; Victoria S Meadows
Journal:  Astrobiology       Date:  2017-11-30       Impact factor: 4.335

2.  The organic Solar System.

Authors:  Bruce C Gibb
Journal:  Nat Chem       Date:  2015-05       Impact factor: 24.427

3.  Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan.

Authors:  Nicholas A Teanby; Patrick G J Irwin; Conor A Nixon; Remco de Kok; Sandrine Vinatier; Athena Coustenis; Elliot Sefton-Nash; Simon B Calcutt; F Michael Flasar
Journal:  Nature       Date:  2012-11-29       Impact factor: 49.962

4.  Aerosol growth in Titan's ionosphere.

Authors:  Panayotis Lavvas; Roger V Yelle; Tommi Koskinen; Axel Bazin; Véronique Vuitton; Erik Vigren; Marina Galand; Anne Wellbrock; Andrew J Coates; Jan-Erik Wahlund; Frank J Crary; Darci Snowden
Journal:  Proc Natl Acad Sci U S A       Date:  2013-02-04       Impact factor: 11.205

5.  A Pilot Study of Ion - Molecule Reactions at Temperatures Relevant to the Atmosphere of Titan.

Authors:  Illia Zymak; Ján Žabka; Miroslav Polášek; Patrik Španěl; David Smith
Journal:  Orig Life Evol Biosph       Date:  2016-04-23       Impact factor: 1.950

6.  The Pale Orange Dot: The Spectrum and Habitability of Hazy Archean Earth.

Authors:  Giada Arney; Shawn D Domagal-Goldman; Victoria S Meadows; Eric T Wolf; Edward Schwieterman; Benjamin Charnay; Mark Claire; Eric Hébrard; Melissa G Trainer
Journal:  Astrobiology       Date:  2016-10-28       Impact factor: 4.335

7.  Protein Stability in Titan's Subsurface Water Ocean.

Authors:  Kyle P Martin; Shannon M MacKenzie; Jason W Barnes; F Marty Ytreberg
Journal:  Astrobiology       Date:  2019-11-15       Impact factor: 4.335

8.  Formation of nitrogenated organic aerosols in the Titan upper atmosphere.

Authors:  Hiroshi Imanaka; Mark A Smith
Journal:  Proc Natl Acad Sci U S A       Date:  2010-07-02       Impact factor: 11.205

9.  Modeling Repeated M Dwarf Flaring at an Earth-like Planet in the Habitable Zone: Atmospheric Effects for an Unmagnetized Planet.

Authors:  Matt A Tilley; Antígona Segura; Victoria Meadows; Suzanne Hawley; James Davenport
Journal:  Astrobiology       Date:  2018-08-02       Impact factor: 4.335

10.  Direct functionalization of C-H bonds by electrophilic anions.

Authors:  Jonas Warneke; Martin Mayer; Markus Rohdenburg; Xin Ma; Judy K Y Liu; Max Grellmann; Sreekanta Debnath; Vladimir A Azov; Edoardo Apra; Robert P Young; Carsten Jenne; Grant E Johnson; Hilkka I Kenttämaa; Knut R Asmis; Julia Laskin
Journal:  Proc Natl Acad Sci U S A       Date:  2020-09-02       Impact factor: 11.205

View more

北京卡尤迪生物科技股份有限公司 © 2022-2023.