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'Superflares' may make it hard for life to thrive on Earth's nearest exoplanet

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Artist's illustration of a powerful flare erupting from the red dwarf star Proxima Centauri.

Artist's illustration of a powerful flare erupting from the red dwarf star Proxima Centauri.  (Roberto Molar Candanosa/Carnegie Institution for Science, NASA/SDO, NASA/JPL)

The nearest exoplanet to Earth may get hit hard by damaging ultraviolet radiation, making it tough for life to survive there, a new study suggests.

That planet, the roughly Earth-mass Proxima b, circles the small, dim star Proxima Centauri, which lies just 4.2 light-years from Earth. And Proxima b orbits in its host's star "habitable zone" — the just-right range of distances where liquid water could theoretically exist on a world's surface. 

But there's a lot more to habitability than just being in the habitable zone, as the new study indicates. In it, a team of researchers analyzing observations by the Evryscope, an array of small telescopes at the Cerro Tololo Inter-American Observatory in the Chilean Andes, report that Proxima Centauri fired off a powerful "superflare" whose light made it to Earth's neighborhood in March 2016. [Proxima b: Closest Earth-Like Planet Discovery in Pictures]

The outburst was 10 times more energetic than any previously observed Proxima Centauri flare, and it briefly boosted the star's brightness by a factor of 68, study team members said. In the flare's immediate aftermath, observers under dark skies would have been able to see the star with the naked eye, which is pretty much unheard of for "red dwarfs" such as Proxima Centauri.

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The Evryscope also spotted 23 less-powerful Proxima Centauri flares over the past two years, according to the study. Based on these observations, the researchers calculated that the red dwarf probably blasts out superflares at least five times per year.

Such activity likely has a profound effect on Proxima b and its atmosphere, the team further found. The team's computer-modeling work suggested that Proxima Centauri's repeated flaring would reduce concentrations of UV-blocking ozone in an Earth-like atmosphere by 90 percent in just five years, and would strip the stuff out of the air completely in a few hundred thousand years. (This isn't to imply that Proxima b has, or ever had, an Earth-like atmosphere; nothing is known about the exoplanet's putative air.)

The UV light generated by the March 2016 superflare "therefore reached the surface with about 100 times the intensity required to kill simple UV-hardy microorganisms, suggesting that life would struggle to survive in the areas of Proxima b exposed to these flares," the team wrote in the new study, which has been submitted to The Astrophysical Journal. (You can read it for free at the online preprint site arXiv.org.)

The new results further bolster a growing sense among astronomers and astrobiologists that radiation could pose a major hurdle to the establishment and evolution of life on Proxima b and other planets circling red dwarfs (which are also known as M dwarfs). Previous studies, for example, have suggested that flares might completely strip away the atmospheres of such worlds over time, leaving their surfaces bare and exposed.

Such dangers aren't as high for possibly habitable worlds around sun-like stars, which tend not to be so active. Also, because sun-like stars are hotter than red dwarfs, their habitable zones are farther away — meaning potentially life-supporting worlds don't get hammered as hard by stellar eruptions.

Still, we shouldn't write off red-dwarf systems as possible abodes of life, said Ward Howard, the lead author of the new study. He cited the lack of detailed knowledge about such planetary systems, as well as the toughness and tenacity of "extremophile" organisms here on Earth, which have surprised researchers time and again.

Researchers "should be careful not to go beyond what we can actually compute and study and measure and observe right now," Howard, a graduate student at the University of North Carolina, told Space.com. "I don't think we can say that there is not life around M-dwarf stars, given the current state of the field."

Originally published on Space.com.

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