Abstract
Venus and Titan are both slowly-rotating, approximately Earth-sized bodies with cloudy, dynamic atmospheres. Each has a complex climate system, even less well understood than the terrestrial equivalent, and the processes that appear to maintain the climate near the surface on both bodies have interesting similarities and differences with each other and with the Earth. By considering these factors and their possible evolution with the aid of elementary climate models, some interesting, albeit tentative, conclusions can be reached concerning the stability of climate on Earth-like planets, and the likely nature of past and future climate change.
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References
Adamcik, J. A., and Draper, A. L.: 1963, ‘The temperature dependence of the Urey Equilibrium and the problem of the carbon dioxide content of the atmosphere of Venus’, Plan. Sp. Sc. 11, 1303–1307.
Bullock, M. A., and Grinspoon, D. G.: 1996, ‘The stability of climate on Venus’, J. Geophys. Res. 101, 7521–7529.
Carlson, R. W., Kamp, L., Baines, K., Pollack, J. B., Grinspoon D., Encrenaz Th., Drossart, P., and Taylor, F. W.: 1993, ‘Variations in Venus cloud-particle properties: A new view of Venus’s cloud morphology as observed by the Galileo near infrared mapping spectrometer’, Plan. Sp. Sc. 41, 477–486.
Esposito, L.W.: 1984, ‘Sulfur dioxide: Episodic injection shows evidence for active Venus volcanism’, Science 223, 1072–1074.
Fulchignoni, M., Ferri, F. et al.: 2005, ‘In situ measurements of the physical characteristics of Titan’s environment’, Nature Online, 30 November 2005.
Goody, R. M., and Yung, Y. L.: 1989, Atmospheric Radiation, Oxford University Press. G
Hashimoto, G. L., and Abe, Y.: 2005, ‘Climate control on Venus: Comparison of the carbonate and pyrite models’, Plan. Sp. Sc. 53, 839–848.
Hashimoto, G. L., Abe, Y., and Sasaki, S.: 1997, ‘CO2 amount on Venus constrained by a criterion of topographic-greenhouse instability’, Geophys. Res. Lett. 24, 289–292.
Knollenberg, R. G., and Hunten, D. M.: 1980, ‘The microphysics of the clouds of Venus: Results of the Pioneer Venus particle size spectrometer experiments’, J. Geophys. Res. 85, 8039–8058.
Lorenz, R. D., McKay C. P., and Lunine J. I.: 1997a, ‘Photochemically-driven collapse of Titan’s atmosphere’, Science 275, 642–644.
Lorenz, R. D., Lunine, J. I., and McKay, C. P.: 1997b, ‘Titan under a red giant sun: A new kind of “Habitable” world’, Geophys. Res. Lett. 24, 2905–2908.
Lorenz, R. D., McKay C. P., and Lunine J. I.: 1999, ‘Analytic investigation of climate stability on Titan: Sensitivity to volatile inventory’, Plan. Sp. Sc. 47, 1503–1515.
McKay, C. P., Pollack, J. B., and Courtin, R.: 1989, ‘The thermal structure of Titan’s atmosphere’, Icarus 80, 23–53.
Nimmo, F., and McKenzie, D.: 1998, ‘Volcanism and tectonics on Venus’, Ann. Rev. Earth Plan. Sc. 26, 23–51.
Taylor, F. W.: 2005, Elementary Climate Physics, Oxford University Press.
Urey, H. C.: 1952, The Planets, Yale University Press, New Haven.
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Taylor, F.W. (2007). Climate Variability on Venus and Titan. In: Calisesi, Y., Bonnet, R.M., Gray, L., Langen, J., Lockwood, M. (eds) Solar Variability and Planetary Climates. Space Sciences Series of ISSI, vol 23. Springer, New York, NY. https://doi.org/10.1007/978-0-387-48341-2_36
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DOI: https://doi.org/10.1007/978-0-387-48341-2_36
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