Bedoukian   RussellIPM   RussellIPM   Piezoelectric Micro-Sprayer


Home
Animal Taxa
Plant Taxa
Semiochemicals
Floral Compounds
Semiochemical Detail
Semiochemicals & Taxa
Synthesis
Control
Invasive spp.
References

Abstract

Guide

Alphascents
Pherobio
InsectScience
E-Econex
Counterpart-Semiochemicals
Print
Email to a Friend
Kindly Donate for The Pherobase

« Previous AbstractPlants-nematodes-microbes crosstalk within soil: A trade-off among friends or foes    Next Abstract[Visualization of fruit scent using photoluminescence] »

Adv Space Res


Title:The organic aerosols of Titan
Author(s):Khare BN; Sagan C; Thompson WR; Arakawa ET; Suits F; Callcott TA; Williams MW; Shrader S; Ogino H; Willingham TO; Nagy B;
Address:"Laboratory for Planetary Studies, Cornell University, Ithaca, NY, USA"
Journal Title:Adv Space Res
Year:1984
Volume:4
Issue:12
Page Number:59 - 68
DOI: 10.1016/0273-1177(84)90545-3
ISSN/ISBN:0273-1177 (Print) 0273-1177 (Linking)
Abstract:"A dark reddish organic solid, called tholin, is synthesized from simulated Titanian atmospheres by irradiation with high energy electrons in a plasma discharge. The visible reflection spectrum of this tholin is found to be similar to that of high altitude aerosols responsible for the albedo and reddish color of Titan. The real (n) and imaginary (k) parts of the complex refractive index of thin films of Titan tholin prepared by continuous D.C. discharge through a 0.9 N2/0.1 CH4 gas mixture at 0.2 mb is determined from x-ray to microwave frequencies. Values of n (approximately equal to 1.65) and k (approximately equal to 0.004 to 0.08) in the visible are consistent with deductions made by ground-based and spaceborne observations of Titan. Many infrared absorption features are present in k (lambda), including the 4.6 micrometers nitrile band. Molecular analysis of the volatile component of this tholin was performed by sequential and non-sequential pyrolytic gas chromatography/mass spectrometry. More than one hundred organic compounds are released; tentative identifications include saturated and unsaturated aliphatic hydrocarbons, substituted polycyclic aromatics, nitriles, amines, pyrroles, pyrazines, pyridines, pyrimidines, and the purine, adenine. In addition, acid hydrolysis produces a racemic mixture of biological and non-biological amino acids. Many of these molecules are implicated in the origin of life on Earth, suggesting Titan as a contemporary laboratory environment for prebiological organic chemistry on a planetary scale"
Keywords:"Aerosols/analysis/*chemistry Astronomy/instrumentation/methods *Atmosphere *Extraterrestrial Environment Gas Chromatography-Mass Spectrometry Hydrolysis Methane/chemistry *Models, Chemical Nitrogen/chemistry Origin of Life Polymers/analysis/*chemistry *Sa;"
Notes:"MedlineKhare, B N Sagan, C Thompson, W R Arakawa, E T Suits, F Callcott, T A Williams, M W Shrader, S Ogino, H Willingham, T O Nagy, B eng DE-AC05-84-OR21400/DE/NIDCR NIH HHS/ Research Support, U.S. Gov't, Non-P.H.S. England 1984/01/01 Adv Space Res. 1984; 4(12):59-68. doi: 10.1016/0273-1177(84)90545-3"

 
Back to top
 
Citation: El-Sayed AM 2024. The Pherobase: Database of Pheromones and Semiochemicals. <http://www.pherobase.com>.
© 2003-2024 The Pherobase - Extensive Database of Pheromones and Semiochemicals. Ashraf M. El-Sayed.
Page created on 26-12-2024