The observability of HCN on Jupiter in the millimeter range

Details The observability of HCN on Jupiter in the millimeter range The observability of HCN on Jupiter in the millimeter range

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...135..365l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 135, no. 2, June 1984, p. 365-370.

Astronomy and Astrophysics

Astronomy

11

Astronomical Spectroscopy, Hydrocyanic Acid, Jupiter (Planet), Planetary Radiation, Radio Astronomy, Jupiter Atmosphere, Millimeter Waves, Molecular Spectroscopy, Jupiter, Hydrogen Cyanide, Spectra, Calculations, Mixing, Photochemistry, Ratios, Observations, Spectroscopy, Atmosphere, Abundance, Infrared, Models, Wavelengths, Physics, Chemistry, Thermochemistry, Source

Scientific paper

Existing spectroscopic data were considered in defining a theoretical model for a synthetic mm-spectrum for Jupiter. The spectrum covered the 700 microns-1 cm region and accounted for absorption by H2, NH3, PH3, HCN and CO as measured by the Voyager IRIS instrument. Nominal profiles were assigned to minor constituents. The results indicate that the HCN J=0, 1, 2 and 3 lines should have sufficient contrast to be observable at mm-wavelengths, provided mountaintop receivers are used for the survey.

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