Space Science Reviews

, Volume 125, Issue 1, pp 445–455

Climate Variability on Venus and Titan


DOI: 10.1007/s11214-006-9077-y

Cite this article as:
Taylor, F.W. Space Sci Rev (2006) 125: 445. doi:10.1007/s11214-006-9077-y


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.



Copyright information

© Springer Science+Business Media, Inc. 2007

Authors and Affiliations

  1. 1.Atmospheric, Oceanic and Planetary PhysicsUniversity of Oxford, Clarendon LaboratoryOxfordEngland