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A significant study has revealed that red dwarf stars can produce stellar flares with far-ultraviolet (far-UV) radiation levels much higher than previously thought. This discovery indicates that the intense UV radiation from these flares could considerably affect the habitability of planets orbiting red dwarf stars. This research, led by current and former astronomers from the University of Hawa by Clarence Oxford
Los Angeles CA (SPX) Aug 06, 2024
A significant study has revealed that red dwarf stars can produce stellar flares with far-ultraviolet (far-UV) radiation levels much higher than previously thought. This discovery indicates that the intense UV radiation from these flares could considerably affect the habitability of planets orbiting red dwarf stars. This research, led by current and former astronomers from the University of Hawai?i Institute for Astronomy (IfA), was recently published in the Monthly Notices of the Royal Astronomical Society.
"Few stars have been thought to generate enough UV radiation through flares to impact planet habitability. Our findings show that many more stars may have this capability," said astronomer Vera Berger, who conducted the study while participating in the Research Experiences for Undergraduates program at IfA, an initiative supported by the National Science Foundation.
Berger and her team utilized archival data from the GALEX space telescope to search for flares among 300,000 nearby stars. GALEX, a now-decommissioned NASA mission, observed most of the sky at near-and far-UV wavelengths from 2003 to 2013. Using new computational techniques, the team extracted novel insights from the data.
"Combining modern computer power with gigabytes of decades-old observations allowed us to search for flares on thousands and thousands of nearby stars," said Michael Tucker, a PhD graduate of IfA and now a postdoctoral fellow at Ohio State University.
Researchers noted that UV radiation from stellar flares could either erode planetary atmospheres, endangering their potential to support life, or contribute to the formation of RNA building blocks, which are essential for the creation of life.
This study challenges existing models of stellar flares and exoplanet habitability, demonstrating that far-UV emission from flares is, on average, three times more energetic than typically assumed, and can reach up to twelve times the expected energy levels.
"A change of three is the same as the difference in UV in the summer from Anchorage, Alaska to Honolulu, where unprotected skin can get a sunburn in less than 10 minutes," said Benjamin J. Shappee, an Associate Astronomer at IfA who mentored Berger.
The exact cause of this stronger far-UV emission remains unclear. The team suggests it might be due to flare radiation being concentrated at specific wavelengths, indicating the presence of atoms like carbon and nitrogen.
"This study has changed the picture of the environments around stars less massive than our Sun, which emit very little UV light outside of flares," said Jason Hinkle, a PhD candidate at IfA who co-authored the study.
According to Berger, now a Churchill Scholar at the University of Cambridge, more data from space telescopes is needed to study the UV light from stars, which is crucial for understanding the source of this emission.
Research Report:Stellar flares are far-ultraviolet luminous
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