The first paper examines how long an atmosphere would survive on Proxima Centauri b, which is only four light-years from Earth and was discovered in 2016. The second paper looks at a type of planet called "water worlds" and questions how long oceans could survive. Because life takes billions of years to evolve, the research has broad implications for understanding of planet habitability.
The researchers concluded that the atmosphere of Proxima Centauri b would only be retained if the pressure from the stellar wind is low and the planet has a magnetic field to deflect the particles. Otherwise, they wrote, over time the stellar wind would strip the planet's atmosphere, which would become so thin that evaporated water in the atmosphere couldn't fall as rain.
"Our results indicate that [Proxima Centauri b] and similar exoplanets are generally not capable of supporting an atmosphere over sufficiently long timescales when the stellar wind pressure is high," Dong said.
Even worse is what happens to the type of star that Proxima Centauri b orbits. The planet is nearby a red dwarf star, which is smaller and produces less energy than our sun. The habitable zone around these stars could change as the star evolves. Specifically, when a red dwarf is young, it is prone to producing high stellar winds. This means a young, nearby planet could lose much of its atmosphere before life has a chance to develop.
"In addition, such close-in planets could also be tidally locked like our moon, with one side always exposed to the star," Dong said. "The resultant weak global magnetic field and the constant bombardment of stellar wind would serve to intensify losses of atmosphere on the star-facing side."
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The second paper asked how the oceans on water worlds would fare under different stellar wind conditions. It considered three scenarios. The first was an environment similar to the winds Earth experiences. The second one considers the stronger stellar winds believed to be present in young stars. And the third evaluates what would happen in the case of a huge "Carrington event" solar storm, which refers to an incident in 1859 on Earth when auroras disrupted telegraph service.
Unfortunately for life prospects, the simulations showed that the stellar wind from young stars would produce greater atmospheric loss on young planets, causing the oceans to dry up. And Carrington-type events — believed to be frequent in these young stars — would cause even more damage.
The researchers said these findings could alter the famous Drake equation, which estimates how many civilizations there might be in the Milky Way. One of the factors in the equation is the number of planets in a given star system with an environment suitable for life. But how that environment is determined to be suitable for life remains a matter of debate.
The authors say more observations, including from the James Webb Space Telescope that NASA will launch in 2019, are necessary to better estimate how many planets could support life.
While the case for life looks pessimistic on Proxima Centauri b, the scientists did note another recently discovery could have a better chance for life. Ross 128b, first announced in November, is just 11 light-years from Earth. It is rocky and in the habitable region of its star. But unlike Proxima Centauri b, the red dwarf star near Ross 128b appears to be quieter, without eruptions that could disrupt life on its surface.
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