Red dwarfs likely host earth-sized planets with water
Computer simulations of the formation of planets orbiting in the habitable zones of low mass stars such as Proxima Centauri by astrophysicists at the University of Bern show that these planets are most likely to be roughly the size of the Earth and to contain large amounts of water.
In August 2016, the announcement of the discovery of a terrestrial exoplanet orbiting in the habitable zone of Proxima Centauri stimulated the imagination of experts and the general public. This star is the nearest star to our sun, though it is 10 times less massive and 500 times less luminous. This discovery, together with the discovery in May 2016 of a similar planet orbiting an even lower-mass star (Trappist-1), convinced astronomers that such red dwarfs (as these low-mass stars are called) might be hosts to a large population of Earth-like planets.
What might these objects look like? What could they be made of? Yann Alibert and Willy Benz at the Swiss NCCR PlanetS and the Center of Space and Habitability (CSH) at the University of Bern carried out the first computer simulations of the formation of planets expected to orbit stars 10 times less massive than the sun.
“Our models succeed in reproducing planets that are similar in terms of mass and period to the ones observed recently,” Alibert says regarding the results of the study, forthcoming as a letter in the journal Astronomy and Astrophysics. “Interestingly, we find that planets in close-in orbits around these type of stars are of small sizes. Typically, they range between 0.5 and 1.5 Earth radii with a peak at about 1.0 Earth radius. Future discoveries will tell if we are correct,” the researcher adds.
Ice at the bottom of the global ocean
In addition, the astrophysicists determined the water content of the planets orbiting their small host stars in the habitable zone. They found that around 90% of the planets harbour more than 10% water. For comparison, the Earth has a fraction of water of only about .02%. The situation could be even more extreme if the protoplanetary disks in which these planets form persist longer than assumed in the models. In any case, these planets would be covered by very deep oceans at the bottom of which, owing to enormous pressure, water would be in form of ice.
Water is required for life as we know it. So could these planets be habitable? “While liquid water is generally thought to be an essential ingredient, too much of a good thing may be bad,” says Willy Benz. In previous studies, the scientists in Bern showed that too much water may prevent the regulation of the surface temperature and destabilize the climate. “But this is the case for the Earth; here, we deal with considerably more exotic planets that might be subjected to a much harsher radiation environment, and/or be synchronous,” he adds.
Following the growth of planetary embryos
To start their calculations, the scientists considered a series of a few hundreds to thousands of identical, low-mass stars, and around each of them, a protoplanetary disk of dust and gas. Planets are formed by accretion of this material. Alibert and Benz assumed that at the beginning, there were 10 planetary embryos in each disk with an initial mass equal to the mass of the moon. In a few day’s computer time for each system, the model calculated how these randomly located embryos grew and migrated. What kind of planets are formed depends on the structure and evolution of the protoplanetary disks.
“Habitable or not, the study of planets orbiting very low-mass stars will likely bring exciting new results, improving our knowledge of planet formation, evolution, and potential habitability,” summarizes Benz. Because these stars are considerably less luminous than the sun, planets can be much closer to their stars before the surface temperature becomes too high for liquid water to exist. Considering that this type of star also represents the overwhelming majority of stars in the solar neighborhood and that close-in planets are presently easier to detect and study, it is easy to understand why the existence of this population of Earth-like planets is of importance.
More information: University of Bern
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