On the thermal structure of Uranus from infrared measurements

Details On the thermal structure of Uranus from infrared measurements On the thermal structure of Uranus from infrared measurements

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....63...97c&link_type=abstract

Astronomy and Astrophysics, vol. 63, no. 1-2, Feb. 1978, p. 97-101.

Astronomy and Astrophysics

Astrophysics

6

Infrared Radiation, Planetary Temperature, Stratosphere, Temperature Profiles, Uranus (Planet), Abundance, Atmospheric Models, Convective Flow, Helium, Supersaturation, Temperature Measurement, Uranus, Infrared, Thermal Properties

Scientific paper

Thermal profiles of Uranus are inferred from presently available infrared measurements of this planet, and compared with the radiative-convective equilibrium models of Wallace (1975). Supersaturation of CH4 in the Uranian stratosphere is not required to explain the infrared features of this planet. The effective temperature of the retrieved profiles is 57 plus or minus 2.5 K for a relative hydrogen abundance of 85 percent. There is no evidence of an internal heat source, and a significant enhancement of helium compared with the solar abundance is unlikely.

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