New IR observations of Titan and potential of in-situ atmospheric analysis of the outer planets

Details New IR observations of Titan and potential of in-situ atmospheric analysis of the outer planets New IR observations of Titan and potential of in-situ atmospheric analysis of the outer planets

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974oppt.workq....o&link_type=abstract

In Dynatrend, Inc. Proc. of Outer Planet Probe Technol. Workshop, Sect. 1 through 11 23 p (SEE N75-20358 12-12)

Computer Science

Infrared Spectra, Jupiter Atmosphere, Neptune (Planet), Titan, Uranus (Planet), Abundance, Atmospheric Composition, Carbon, Hydrogen, Methane, Planetary Atmospheres

Scientific paper

Ground based telescopic observations of Titan and outer planet atmospheres are evaluated for their abundances and an effort is made to deduce the various hydrogen-to-carbon ratios. Jupiter and Saturn atmospheres seem to have roughly solar abundances as far as hydrogen and methane are concerned; for Uranus, Titan and Neptune these ratios are way down.

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