Active upper-atmosphere chemistry and dynamics from polar circulation reversal on Titan

• Published in: Nature
• Main Authors: Teanby, Nicholas A., Irwin, Patrick G.J., Nixon, Conor A., De Kok, Remco, Vinatier, Sandrine, Coustenis, Athena, Sefton-Nash, Elliot, Calcutt, Simon B., Flasar, F.M.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2012
• Subjects: Life Science; South Pole; South pole
• Online Access: https://research.wur.nl/en/publications/active-upper-atmosphere-chemistry-and-dynamics-from-polar-circula; https://doi.org/10.1038/nature11611

Saturn's moon Titan has a nitrogen atmosphere comparable to Earth's, with a surface pressure of 1.4 bar. Numerical models reproduce the tropospheric conditions very well but have trouble explaining the observed middle-atmosphere temperatures, composition and winds. The top of the middle-atmosphere circulation has been thought to lie at an altitude of 450 to 500 kilometres, where there is a layer of haze that appears to be separated from the main haze deck. This 'detached' haze was previously explained as being due to the co-location of peak haze production and the limit of dynamical transport by the circulation's upper branch. Here we report a build-up of trace gases over the south pole approximately two years after observing the 2009 post-equinox circulation reversal, from which we conclude that middle-atmosphere circulation must extend to an altitude of at least 600 kilometres. The primary drivers of this circulation are summer-hemisphere heating of haze by absorption of solar radiation and winter-hemisphere cooling due to infrared emission by haze and trace gases; our results therefore imply that these effects are important well into the thermosphere (altitudes higher than 500 kilometres). This requires both active upper-atmosphere chemistry, consistent with the detection of high-complexity molecules and ions at altitudes greater than 950 kilometres, and an alternative explanation for the detached haze, such as a transition in haze particle growth from monomers to fractal structures.