Catholic University of Leuven, Belgium | 2016 July 14
[img3=""]http://www.kuleuven.be/english/news/sur ... anet/image[/img3][hr][/hr]KU Leuven astronomers have shown that the interaction between the surface and the atmosphere of an exoplanet has major consequences for the temperature on the planet. This temperature, in turn, is a crucial element in the quest for habitable planets outside our Solar System.
In the quest for habitable planets outside our Solar System – also known as exoplanets – astronomers are currently focusing on rocky planets that don’t look like Earth. These planets orbit so-called M dwarfs – stars that are smaller than our Sun. In our universe, there are many more M dwarfs than there are sun-like stars, making it more likely that astronomers will discover the first habitable exoplanet around an M dwarf. Most planets orbiting these M dwarfs always face their star with the same side. As a result, they have permanent day and night sides. The day side is too hot to make life possible, while the night side is too cold.
Last year, KU Leuven researchers Ludmila Carone, Professor Rony Keppens, and Professor Leen Decin already showed that planets with permanent day sides may still be habitable depending on their 'air conditioning' system. Two out of three possible ‘air conditioning’ systems on these exoplanets use the cold air of the night side to cool down the day side. And with the right atmosphere and temperature, planets with permanent day and night sides are potentially habitable. ...
But this is not always the case: on the equator of many of these rocky planets, a strong air current in the upper layers of the atmosphere interferes with the circulation of hot air to the night side. The ‘air conditioning’ system stops working, and the planet becomes uninhabitable because the temperatures are too extreme. ...
Connecting the Dots III: Night Side Cooling and Surface Friction Affect Climates
of Tidally Locked Terrestrial Planets - Ludmila Carone, Rony Keppens, Leen Decin
- Monthly Notices of the RAS 461(2):1981 (2016 Sep 11) DOI: 10.1093/mnras/stw1265
arXiv.org > astro-ph > arXiv:1605.09545 > 31 May 2016