A series of megaflares unleashed earlier this year by a nearby red dwarf has astronomers rethinking just what these small, dim stars are capable of.

On April 23, NASA's Swift satellite spotted the enormous star flare coming from DG Canum Venaticorum (DG CVn), a system of two red dwarfs located about 60 light-years from Earth. The eruption put to shame anything ever seen on the sun, whose strong flares are classified into three categories, with C flares being the weakest, M of medium strength and X the most powerful.

"The biggest flare we've ever seen from the sun occurred in November 2003 and is rated as X45," Stephen Drake, an astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Maryland, said in a statement. "The flare on DG CVn, if viewed from a planet the same distance as Earth is from the sun, would have been roughly 10,000 times greater than this, with a rating of about X100,000." [Biggest Solar Flares of 2014: Sun Storm Photos]

Artist's concept showing DG CVn — a binary system consisting of two red dwarf stars — unleashing a series of powerful flares seen by NASA's Swift spacecraft on April 23, 2014.
Artist's concept showing DG CVn — a binary system consisting of two red dwarf stars — unleashing a series of powerful flares seen by NASA's Swift spacecraft on April 23, 2014.
Credit: NASA's Goddard Space Flight Center/S. Wiessinger

For a few minutes, the superflare's X-ray brightness outshone both stars' total luminosity in all wavelengths, researchers said. The eruption's temperature reached 360 million degrees Fahrenheit (200 million degrees Celsius) — about 13 times hotter than the sun's core.

But DG CVn wasn't done yet, firing off a number of other flares over the next 11 days, with each one being a bit weaker than the last. X-ray emission from the system finally returned to baseline levels 20 days after the April 23 event.

DG CVn's sustained activity surprised scientists.

"We used to think major flaring episodes from red dwarfs lasted no more than a day, but Swift detected at least seven powerful eruptions over a period of about two weeks," said Drake, who gave a presentation about the DG CVn superflare in August at a meeting of the American Astronomical Society’s High Energy Astrophysics Division. "This was a very complex event."

Both of the stars in the DG CVn system are about one-third as massive as the sun. They orbit about 3 astronomical units from each other — too close for Swift to tell which one of them was responsible for the big flares this year. (One astronomical unit, or AU, is the average distance from Earth to the sun — about 93 million miles, or 150 million kilometers).

Though they look serene and silent from our vantage on Earth, stars are actually roiling balls of violent plasma. Test your stellar smarts with this quiz.
Open Star Cluster Messier 50
0 of 10 questions complete
Star Quiz: Test Your Stellar Smarts
Though they look serene and silent from our vantage on Earth, stars are actually roiling balls of violent plasma. Test your stellar smarts with this quiz.
Open Star Cluster Messier 50
0 of questions complete
The DG CVn stars complete one rotation in less than a day, compared to about 25 days for the sun. The dwarfs' rotational speed helps explain how they are capable of such powerful flaring, researchers said: Flares erupt when a star's twisted magnetic fields reconnect, and rapid spin amps these fields up.

The sun may once have blasted out megaflares, too. A star's rotational speed decreases as it ages, and our sun is middle-aged at about 5 billion years old. The DG CVn stars are just 30 million years old or so, researchers said.

Follow Mike Wall on Twitter @michaeldwall and Google+. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.