Monodeurated methane in the outer solar system. 2. Its detection on Uranus at 1.6 microns

Details Monodeurated methane in the outer solar system. 2. Its detection on Uranus at 1.6 microns Monodeurated methane in the outer solar system. 2. Its detection on Uranus at 1.6 microns

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stin...8527782d&link_type=abstract

Monodeurated methane in the outer solar system. 2. Its detection on Uranus at 1.6 microns

Other

Atmospheric Models, Deuterium, Deuterium Compounds, Jupiter Atmosphere, Methane, Uranus Atmosphere, Fourier Transformation, Mixing, Spectrometers, Spectroscopy, Spectrum Analysis

Scientific paper

Deuterium in the atmosphere of Uranus has been studied only via measurements of the exceedingly weak dipole lines of hydrogen-deuteride (HD) seen in the visible region of the spectrum. The other sensitive indicator of deuterium in the outer solar system is monodeuterated methane (CH3D) but the two bands normally used ot study this molecule, NU2 near 2200 1/cm and NU6 near 1161 1/cm, have not been detected in Uranus.

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