Correction: A follow-up paper by Barth & Stern (2018) has shown that the evidence for periodic light variations presented in Dorn-Wallenstein et al. (2017) and publicized in this press release is not, in fact, significant. Although a supermassive black hole behind M31 has been discovered, the claim that a pair of supermassive black holes was detected can no longer be made.
Editor’s Note: Honest errors such as this are part of the scientific process, especially on the frontiers of discovery. To quote Nobel laureate Frank Wilczek, “If you don’t make mistakes, you’re not working on hard enough problems. And that’s a big mistake.”
Using data from NASA’s Chandra X-ray Observatory and ground-based optical telescopes, an intriguing source has been discovered in the nearby Andromeda galaxy. Previously thought to be part of the Milky Way’s neighbor galaxy, the new research shows this source is actually a very distant object 2.6 billion light years away.
- A pair of supermassive black holes have “photobombed” the Andromeda galaxy.
- Astronomers previously thought this source, known as J0045+41, was part of Andromeda, which is about 2.5 million light-years from Earth.
- New data from Chandra and ground-based optical data reveal J0045+41 is actually 1,000 times more distant.
- The latest information suggests J0045+41 contains a pair of giant black holes orbiting one another extremely closely.
It seems like even black holes can’t resist the temptation to insert themselves unannounced into photographs. A cosmic photobomb found as a background object in images of the nearby Andromeda galaxy has revealed what could be the most tightly coupled pair of supermassive black holes ever seen.
Astronomers made this remarkable discovery using X-ray data from NASA’s Chandra X-ray Observatory and optical data from ground-based telescopes, Gemini-North in Hawaii, and the Caltech’s Palomar Transient Factory in California.
This unusual source, called LGGS J004527.30+413254.3 (J0045+41 for short), was seen in optical and X-ray images of Andromeda, also known as M31. Until recently, scientists thought J0045+41 was an object within M31, a large spiral galaxy located relatively nearby at a distance of about 2.5 million light-years from Earth. The new data, however, revealed that J0045+41 was actually at a much greater distance, around 2.6 billion light-years from Earth.
“We were looking for a special type of star in M31 and thought we had found one,” said Trevor Dorn-Wallenstein of the University of Washington in Seattle, WA, who led the paper describing this discovery. “We were surprised and excited to find something far stranger!”
Even more intriguing than the large distance of J0045+41 is that it likely contains a pair of giant black holes in close orbit around each other. The estimated total mass of these two supermassive black holes is about two hundred million times the mass of our Sun.
Previously, a different team of astronomers had seen periodic variations in the optical light from J0045+41, and, believing it to be a member of M31, classified it as a pair of stars that orbited around each other about once every 80 days.
The intensity of the X-ray source observed by Chandra revealed this original classification was incorrect. Rather, J0045+41 had to be either a binary system in M31 containing a neutron star or black hole that is pulling material from a companion — the sort of system Dorn-Wallenstein was originally searching for in M31 — or a much more massive and distant system that contains at least one rapidly growing supermassive black hole.
However, a spectrum from the Gemini-North telescope taken by the University of Washington team showed that J0045+41 must host at least one supermassive black hole and allowed the researchers to estimate the distance. The spectrum also provided possible evidence that a second black hole was present in J0045+41 and moving at a different velocity from the first, as expected if the two black holes are orbiting each other.
The team then used optical data from the Palomar Transient Factory to search for periodic variations in the light from J0045+41. They found several periods in J0045+41, including ones at about 80 and 320 days. The ratio between these periods matches that predicted by theoretical work on the dynamics of two giant black holes orbiting each other.
“This is the first time such strong evidence has been found for a pair of orbiting giant black holes,” said co-author Emily Levesque of the University of Washington.
The researchers estimate that the two putative black holes orbit each other with a separation of only a few hundred times the distance between the Earth and the Sun. This corresponds to less than one hundredth of a light year. By comparison, the nearest star to our Sun is about four light years away.
Such a system could be formed as a consequence of the merger, billions of years earlier, of two galaxies that each contained a supermassive black hole. At their current close separation, the two black holes are inevitably being drawn closer together as they emit gravitational waves.
“We’re unable to pinpoint exactly how much mass each of these black holes contains,” said co-author John Ruan, also of the University of Washington. “Depending on that, we think this pair will collide and merge into one black hole in as little as 350 years or as much as 360,000 years.”
If J0045+41 indeed contains two closely orbiting black holes it will be emitting gravitational waves, however the signal would not be detectable with LIGO and Virgo. These ground-based facilities have detected the mergers of stellar-mass black holes weighing no more than about 60 Suns and, very recently, one between two neutron stars.
“Supermassive black hole mergers occur in slow motion compared to stellar-mass black holes”, said Dorn-Wallenstein. “The much slower changes in the gravitational waves from a system like J0045+41 can be best detected by a different type of gravitational wave facility called a Pulsar Timing Array.”
Reference: “A Mote in Andromeda’s Disk: a Misidentified Periodic AGN Behind M31” by Trevor Dorn-Wallenstein1, Emily M. Levesque1, and John J. Ruan, 20 November 2017, The Astrophysical Journal.