The pair is also unique in being one of a few known sources of gravitational waves—ripples in space and time—that will be picked up by the future European space mission LISA (Laser Interferometer Space Antenna), which is expected to launch in 2034. LISA, in which NASA plays a role, will be similar to the National Science Foundation's ground-based LIGO (Laser Interferometer Gravitational-wave Observatory), which made history in 2015 by making the first direct detection of gravitational waves from a pair of colliding black holes. But LISA will detect the waves from space at lower frequencies.

"These two white dwarfs are merging because they are emitting gravitational waves. Within a week of LISA turning on, it should pick up the gravitational waves from this system," says co-author Tom Prince, the Ira S. Bowen Professor of Physics at Caltech and a senior research scientist at JPL. "LISA will find tens of thousands of binary systems in our galaxy like this one, but so far we only know of a few. And this binary-star system is one of the best characterized yet due to its eclipsing nature."

A Rapid Blinking in the Night Sky

The rare object was spotted by ZTF, a large 576-megapixel camera residing on the Samuel Oschin Telescope at Palomar, that rapidly scans the entire sky every three nights and the bulk of the plane of the Milky Way every night. Burdge found ZTF J1539+5027 by running a computer program that tracked 10 million cosmic objects, looking for changes over a three-month span. Once he found candidate objects with ZTF, Burdge used the National Optical Astronomy Observatory's Kitt Peak National Observatory, which is funded by the National Science Foundation (NSF), to follow up and find the most promising candidates.

"This pair really stuck out because the signal repeats so often and in such a predictable way," says Burdge, who is a member of the ZTF team at Caltech. "People haven't been able to systematically search for things that change on minute-time scales before. ZTF lets us do this because its camera is huge and it can easily take pictures across the sky and then come back and repeat."

ZTF is funded by the NSF and an international collaboration of partners. Additional support comes from NASA, the Heising-Simons Foundation, members of the Space Innovation Council at Caltech, and Caltech itself. Follow-up observations made with the 200-inch Hale Telescope at Palomar Observatory and the W. M. Keck Observatory helped refine measurements of the newfound system.

"Only months after coming online, ZTF astronomers have detected white dwarfs orbiting each other at a record pace," says NSF assistant director for mathematical and physical sciences Anne Kinney. "It's a discovery that will greatly improve our understanding of these systems, and it's a taste of surprises yet to come."

A Tangled Pair

The white dwarfs began their lives as stars like our sun, except they were bound together as a tight-knit pair. As the stars aged, they swelled up into red giants, though not at the same time. Over time, the swollen stars shed their outer layers, leaving behind two dead stars—the white dwarfs.

"Sometimes these binary white dwarfs merge into one star, and other times the orbit widens as the lighter white dwarf is gradually shredded by the heavier one," says co-author James (Jim) Fuller, an assistant professor of theoretical astrophysics at Caltech. "We're not sure what will happen in this case, but finding more such systems will tell us how often these stars survive their close encounters."

Another mystery the researchers hope to answer in the future involves the temperature of the hotter white dwarf, which is estimated to be 50,000 Celsius, or nine times hotter than the sun. This white dwarf is thought to be so hot because it is starting to "feed" off its companion and pull material onto it, a process that heats material to sizzling-hot temperatures. But this feeding, or "accretion" process, is usually associated with X-rays, and the researchers are not seeing any.

"It's strange that we aren't seeing X-rays in this system. One possibility is that the accretion spots on the white dwarf—the areas the material is falling on—are bigger than what is typical, and this could result in the emission of ultraviolet light and optical light instead of X-rays," says Burdge.

The team says that the white-dwarf duo, located nearly 8,000 light-years away in the Boötes constellation, should keep blinking in the night sky for a hundred thousand years to come. Amateur astronomers may be able to even see the pair as one spot on the sky, flashing every seven minutes, with the help of a telescope at least one meter in size.

The study, titled, "General Relativistic Orbital Decay in a Seven-Minute-Orbital-Period Eclipsing Binary System," was funded by the ZTF collaboration. Other Caltech authors include Michael Coughlin, David and Ellen Lee Postdoctoral Scholar in Physics; Matthew Graham, research professor of astronomy; Jan van Roestel, postdoctoral scholar in astronomy; Dmitry Duev, research scientist; George Helou, research professor of physics and executive director of IPAC; Ashish Mahabal, senior computational and data scientist; and Shri Kulkarni, George Ellery Hale Professor of Astronomy and Planetary Science. Other contributing institutions include the Kavli Institute for Theoretical Physics, the University of Washington, UC Santa Barbara, the University of Wisconsin-Milwaukee, the Humboldt University of Berlin, and the Weizmann Institute of Science.