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Seminar über Troposphärenforschung (IMK-TRO)

Ansprechpartner: Prof. Dr. Ch. Kottmeier,   PD Dr. M. Kunz,  Prof. Dr. C. Hoose, Prof. Dr. P. Knippertz, Prof. Dr. A. Fink , Prof. Dr. J. Pinto


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Climate dynamics of lava planets
06.02.2018, 15:00 bis 16:00
KIT Campus Nord, IMK
Gebäude 435, Raum 2.05

Lava planets are rocky planets in orbits sufficiently close to their host stars that they are tide locked with a substellar temperature above the liquidus of typical silicate minerals. Such planets have a permanent dayside magma ocean.  Corot 7b was the first lava planet to have been discovered, but many more have entered the catalogue since, of which the best characterized so far is 55 Cancri e. I will discuss the atmospheric dynamics of lava planets, with particular emphasis on 55 Cancri e, for which case we conclude that the best fit to the observed phase curve demands a moderately thick non condensible background atmosphere rather than a thin mineral vapor atmosphere localized to the dayside. Our earlier work on this problem made use of idealized gray-gas radiation with diagnostic clouds. In this lecture I will present updated results with real-gas radiative transfer for CO dominated atmospheres, and simulations incorporating multi species mineral vapor cloud physics. As in our idealized simulations, the dayside is largely clear-sky, with clouds forming only on the nightside. The simulation exhibits a rich variety of clouds, which will have a strong effect on the thermal emission signature.

Diese Veranstaltung ist Teil der Reihe Karlsruher Meteorologisches Kolloquium
Prof. Raymond Pierrehumbert

University of Oxford
Department of Physics
Institut für Meteorologie und Klimaforschung (IMK-AAF)
Hermann von Helmholtzplatz 1
76344 Eggenstein-Leopoldshafen
Tel: 0721-608-23943
Fax: 0721-608-24332
E-Mail:susanne bolzZtp2∂kit edu
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