A One-Of-A-Kind Star Found to Change Over Decades

“One model of this system predicts long-term variations in the way the two stars interact. It was not known what the time scale of these changes might be — whether 20 to 200 years. By looking at the K2 and archival data, we were able to show that in addition to hourly changes in the system, there are variations occurring over decades,” said Peter Garnavich, professor and department chair of astrophysics and cosmology physics at Notre Dame.

A white dwarf is a very dense remnant of a star like the sun. When a solar-like star runs out of energy, gravity compresses its core to about the size of the Earth but with a mass 300,000 times higher. A teaspoon-sized piece of a white dwarf would weigh about 15 tons. The compression of the star can also amplify its magnetic field strength and its spin rate.

The unique system became famous in 2016 when researchers in England discovered that AR Scorpii, believed to be a mundane solitary star, was actually a rapidly varying binary. The system is remarkable as the white dwarf spins on its axis at an incredibly fast rate, causing flashes in luminosity every two minutes. The amplitude of the flashes varies over the 3.5-hour orbital period, something no other white dwarf binary system is known to do.

“We found that back 12 years ago, AR Scorpii’s peak brightness came a bit later in its orbit than it does now,” said Colin Littlefield, research associate working with Garnavich. “This does not solve the mystery, but it is another piece to the puzzle that is AR Scorpii.”

The team at Notre Dame has been observing the system with the Sarah L. Krizmanich Telescope at the University’s Jordan Hall of Science, and they plan to publish those results in an upcoming paper.

Co-authors of the study include Notre Dame Naughton Fellow Mark Kennedy, Paul Callanan at University College Cork, Benjamin Shappee at Carnegie Observatories and Thomas Holoien at The Ohio State University.

Research was funded in part by NASA.

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