- How hospitable are red dwarf stars, the most common and long-lasting stars in our Galaxy?
- Researchers used Chandra and Hubble data to look at the intensity and frequency of high-energy flares from one nearby red dwarf.
- Barnard’s Star is one of the closest stars to Earth at a distance of only 6 light years.
- At its age of 10 billion years old, Barnard’s Star is still very active and potentially destructive for the atmospheres of any planets orbiting around it.
A research study using data from NASA’s Chandra X-ray Observatory and Hubble Space Telescope gives new insight into an important question: how habitable are planets that orbit the most common type of stars in the Galaxy? The target of the new study is Barnard’s Star, which is one of the closest stars to Earth at a distance of just 6 light-years. Barnard’s Star is a red dwarf, a small star that slowly burns through its fuel supply and can last much longer than medium-sized stars like our Sun. It is about 10 billion years old, making it twice the age of the Sun.
The authors used Barnard’s Star as a case study to learn how flares from an old red dwarf might affect any planets orbiting it. The artist’s illustration t the top of this page depicts an old red dwarf like Barnard’s Star (right) and an orbiting, rocky planet (left).
The research team’s Chandra observations of Barnard’s Star taken in June 2019 uncovered one X-ray flare and their Hubble observations taken in March 2019 revealed two ultraviolet high-energy flares (shown in the graphic above). Both observations were about seven hours long and both plots show X-ray or ultraviolet brightness extending down to zero. Based on the length of the flares and of the observations, the authors concluded that Barnard’s Star unleashes potentially destructive flares about 25% of the time.
The team then studied what these results mean for rocky planets orbiting in the habitable zone — where liquid water could exist on their surface — around an old red dwarf like Barnard’s Star. Any atmosphere formed early in the life of a habitable-zone planet was likely to have been eroded away by high-energy radiation from the star during its volatile youth. Later on, however, planet atmospheres might regenerate as the star becomes less active with age. This regeneration process may occur by gases released by impacts of solid material or gases being released by volcanic processes.
However, the onslaught of powerful flares like those reported here, repeatedly occurring over hundreds of millions of years, may erode any regenerated atmospheres on rocky planets in the habitable zone. The illustration shows the atmosphere of the rocky planet being swept away to the left by energetic radiation from flares produced by the red dwarf. This would reduce the chance of these worlds supporting life. The team is currently studying high-energy radiation from many more red dwarfs to determine whether Barnard’s Star is typical.
Reference: “The High-energy Radiation Environment around a 10 Gyr M Dwarf: Habitable at Last?” by Kevin France, Girish Duvvuri, Hilary Egan, Tommi Koskinen, David J. Wilson, Allison Youngblood, Cynthia S. Froning, Alexander Brown, Julián D. Alvarado-Gómez, Zachory K. Berta-Thompson, Jeremy J. Drake, Cecilia Garraffo, Lisa Kaltenegger, Adam F. Kowalski, Jeffrey L. Linsky, R. O. Parke Loyd, Pablo J. D. Mauas, Yamila Miguel, J. Sebastian Pineda, Sarah Rugheimer, P. Christian Schneider, Feng Tian and Mariela Vieytes, 30 October 2020, The Astronomical Journal.
A paper describing these results, led by Kevin France of the University of Colorado at Boulder, appears in the October 30, 2020 issue of The Astronomical Journal. NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science and flight operations from Cambridge and Burlington, Massachusetts.
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