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AGU: Geophysical Research Letters

 

Index Terms

  • Mathematical Geophysics: Nonlinear dynamics
  • Meteorology and Atmospheric Dynamics: Planetary meteorology

Abstract

Titan, Mars and Earth : Entropy production by latitudinal heat transport

Ralph D. Lorenz

Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721‐0092, USA

Jonathan I. Lunine

Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721‐0092, USA

Paul G. Withers

Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721‐0092, USA

Christopher P. McKay

NASA Ames Research Center, Moffett Field, CA 94035, USA

Temperature contrasts between warm tropics and cool high latitudes depends on how efficiently heat is transported by the atmosphere (and oceans) from the tropics. This heat transport is generally assumed to be proportional to atmospheric pressure, but we show with a simple model that this prediction fails by orders of magnitude for Mars and Titan. However, a basic principle, previously postulated for the Earth, does successfully predict the heat flows and zonal temperatures of Mars and Titan. The circulation predicted by this Maximum Entropy Production (MEP) principle is consistent with Titan's observed zonal structure and the winds and CO2 frost cycle on Mars. The principle makes powerful predictions where detailed information is lacking, such as on the early Earth and on possibly habitable extrasolar planets.

Received 13 September 2000; accepted 16 November 2000; .

Citation: Lorenz, R. D., J. I. Lunine, P. G. Withers, and C. P. McKay (2001), Titan, Mars and Earth : Entropy production by latitudinal heat transport, Geophys. Res. Lett., 28(3), 415–418.

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