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Monodeuterated methane in the outer solar system. III - Its abundance of Titan
- 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 :
- Lunar And Planetary Exploration
Subjects
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