A recent study estimates stars like ours produce superflares about once a century by analyzing Kepler data on tens of thousands of Sun-like stars.
Superflares emit about 1032 erg of radiation, or 6.2444 electron volts (eV). These flares cause significant damage to radio communications, power grids, navigation systems, and spacecraft and astronauts.
The Kepler Space Telescope monitored about 100,000 main-sequence stars continuously for years for signs of periodic dips indicating the presence of exoplanets. This same telescope recorded countless solar flares, giving observers plenty of data on stellar activity.
The team analyzed data obtained by Kepler from 56,450 Sun-like stars between 2009 and 2013. They identified 2,889 superflares from 2,527 of the observed stars, producing an average of one superflare per star per century.
Previous surveys found average intervals of a thousand or even ten thousand years, but this study is more precise and sensitive. Nevertheless, it is possible that more violent solar particle events and superflares occurred in the past.
It is unclear whether gigantic flares are always accompanied by coronal mass ejections and what is the relationship between superflares and extreme solar particle events. This requires further investigation.
The new data remind us that even the most extreme solar events are part of the Sun’s natural repertoire, urging caution and regular monitoring.
By 2031, ESA’s Vigil probe, assisted by MPS’s Polarimetric and Magnetic Imager (PHI) instrument, will help monitor the Sun more effectively for reliable forecasting and advanced warning.
While astronomers have not yet determined whether the Sun can produce “superflares”, numerous agencies actively monitor the Sun’s behavior to learn more about its long-term behavior.
Previous surveys had to limit themselves to stars without any close neighbors, making this study the most precise and sensitive to date to determine the exact source of observed flares.