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Monodeuterated methane in the outer solar system. III - Its abundance of Titan

Authors :
De Bergh, C
Chauville, J
Lutz, B. L
Owen, T
Source :
Astrophysical Journal, Part 1. 329
Publication Year :
1988
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1988.

Abstract

The 3nv2 band of CH3D has been detected in spectra of Titan recorded at 1.6 microns with the Fourier transform spectrometer at the 4 m telescope of the Kitt Peak National Observatory. A value of the CH3D/Ch4 mixing ratio is obtained from a comparison between the observed Titan spectra and synthetic spectra. This value is about 2 times higher than the value measured on Uranus (de Bergh et al. 1981, 1986) and about 6 times higher than on Jupiter and on Saturn (Courtin et al. 1984; de Bergh et al.). The value found on Titan for D/H in methane is comparable to the D/H ratio measured in terrestrial H2O.

Subjects

Subjects :
Lunar And Planetary Exploration

Details

Language :
English
ISSN :
0004637X
Volume :
329
Database :
NASA Technical Reports
Journal :
Astrophysical Journal, Part 1
Notes :
NSG-7499, , NGR-33-015-141
Publication Type :
Report
Accession number :
edsnas.19880054390
Document Type :
Report
Full Text :
https://doi.org/10.1086/166439