Sun-like Stars Produce Superflares Roughly Once Per Century
Stellar superflares are energetic outbursts of electromagnetic radiation, similar to solar flares but releasing more energy, up to 1036 erg on main sequence stars.
It is unknown whether the Sun can generate superflares, and if so, how often they might occur. We used photometry from the Kepler space observatory to investigate superflares on other stars with Sun-like fundamental parameters.
We identified 2,889 superflares on 2,527 Sun-like stars, out of 56,450 observed. This detection rate indicates that superflares with energies >1034 erg occur roughly once per century on stars with Sun-like temperature and variability.
The resulting stellar superflare frequency-energy distribution is consistent with an extrapolation of the Sun’s flare distribution to higher energies, so we suggest that both are generated by the same physical mechanism.
Valeriy Vasilyev, Timo Reinhold, Alexander I. Shapiro, Ilya Usoskin, Natalie A. Krivova, Hiroyuki Maehara, Yuta Notsu, Allan Sacha Brun, Sami K. Solanki, Laurent Gizon
Comments: Accepted for publication in Science
Subjects: Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2412.12265 [astro-ph.SR] (or arXiv:2412.12265v1 [astro-ph.SR] for this version)
https://doi.org/10.48550/arXiv.2412.12265
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Journal reference: SCIENCE 12 Dec 2024; Vol 386, Issue 6727, pp. 1301-1305
Related DOI:
https://doi.org/10.1126/science.adl5441
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Submission history
From: Valeriy Vasilyev
[v1] Mon, 16 Dec 2024 19:00:03 UTC (1,151 KB)
https://arxiv.org/abs/2412.12265
Astrobiology,