$^{1}$J. T. Trauger, F. L. Roesler, N. P. Carleton, and W. A. Traub, Astrophys. J. 184, L137 (1973). This work was supported by the NSF Atmospheric Research Section.Author Institution: Department of Physics, University of WisconsinThe ratios of deuterium to hydrogen in the planets constitute important constraints for models of their evolution from the primitive solar nebula. This ratio is most accurately estimated for the major planets from measurements of the $HD/H_{2}$ ratio in their visible atmospheres, since molecular hydrogen predominates and this ratio is least affected among the observed hydrogen bearing molecular species by the poorly known details of the atmospheres. The HD abundance, as first measured by Trauger et al.,$^{1}$ was ...
The abundance of deuterium in giant planet atmospheres provides constraints on the reservoirs of ice...
High resolution spectra of HD and H2 were brought together to derive the D/H ratio for Uranus. The d...
Observations of Jupiter, performed on March 29, 1996, with the Short-Wavelength Spectrometer (SWS) o...
$^{1}$J. T. Trauger, F. L. Roesler, N. P. Carleton, and W. A. Traub, Astrophys. J. 184, L137 (1973)....
A feature was detected at the expected wavelength for the HD R5(0) line in Jupiter's and Uranus' atm...
$^{1}$D. N. Schramm and R. V. Wagoner, Physics Today 27, 41 (1974). $^{2}$R. Beer and F. W. Taylor, ...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
We present new measurements of the deuterium abundance on Jupiter and Saturn, showing evidence that ...
A survey of the abundances of deuterium in planetary atmospheres and small bodies has been carried o...
The D/H ratio is a powerful window into the evolution of atmospheres. Atmospheric escape results los...
The abundance of deuterium in giant planet atmospheres provides constraints on the reservoirs of ice...
High resolution spectra of HD and H2 were brought together to derive the D/H ratio for Uranus. The d...
Observations of Jupiter, performed on March 29, 1996, with the Short-Wavelength Spectrometer (SWS) o...
$^{1}$J. T. Trauger, F. L. Roesler, N. P. Carleton, and W. A. Traub, Astrophys. J. 184, L137 (1973)....
A feature was detected at the expected wavelength for the HD R5(0) line in Jupiter's and Uranus' atm...
$^{1}$D. N. Schramm and R. V. Wagoner, Physics Today 27, 41 (1974). $^{2}$R. Beer and F. W. Taylor, ...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
We present new measurements of the deuterium abundance on Jupiter and Saturn, showing evidence that ...
A survey of the abundances of deuterium in planetary atmospheres and small bodies has been carried o...
The D/H ratio is a powerful window into the evolution of atmospheres. Atmospheric escape results los...
The abundance of deuterium in giant planet atmospheres provides constraints on the reservoirs of ice...
High resolution spectra of HD and H2 were brought together to derive the D/H ratio for Uranus. The d...
Observations of Jupiter, performed on March 29, 1996, with the Short-Wavelength Spectrometer (SWS) o...