Surface Composition Determines Planet's Temperature and Habitability
by Staff Writers
Leuven, Belgium (SPX) Jul 17, 2016
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.
Whether the 'air conditioning' system is actually effective depends on the interaction between the surface of the planet and its atmosphere, Ludmila Carone's new study shows. Carone: "We built hundreds of computer models to examine this interaction. In an ideal situation, the cool air is transported from the night to the day side. On the latter side, the air is gradually heated by the star. This hot air rises to the upper layers of the atmosphere, where it is transported to the night side of the planet again."
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. Ludmila Carone: "Our models show that friction between the surface of the planet and the lower layers of the atmosphere can suppress these strong air currents. When there is a lot of surface friction, the 'air conditioning' system still works."
The KU Leuven researchers created models in which the surface-atmosphere interaction on the exoplanet is the same as on Earth, and models in which there is ten times as much interaction as on Earth. In the latter case, the exoplanets had a more habitable climate. If planets with a well-functioning 'air conditioning' system also have the right atmosphere composition, there's a good chance that these exoplanets are habitable.
"Connecting the Dots III: Night Side Cooling and Surface Friction Affect Climates of Tidally Locked Terrestrial Planets," Ludmila Carone, Rony Keppens and Leen Decin, 2016 Sept. 11, Monthly Notices of the Royal Astronomical Society
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