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Artistic illustration of the centre of OJ 287, in which two black holes orbit ea

Artistic illustration of the centre of OJ 287, in which two black holes orbit each other. Picture: NASA/JPL-Caltech

International research team verifies the validity of the "No Hair" theorem by actual observations

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With the help of NASA’s Spitzer Space Telescope, an international team of researchers has confirmed that the cosmic object OJ 287 is a distant galaxy with a binary system of two supermassive black holes in its centre, which are orbiting each other. With the measurement data that the scientists present in today’s issue of the "Astrophysical Journal Letters" , they also verify the "no-hair" theorem of black holes. Astrophysicists from the Friedrich Schiller University Jena are among the authors of the study.

It took more than 100 years until the existence of gravitational waves predicted by Albert Einstein in 1915 as part of his general theory of relativity was finally proven in an experiment. The first observation of gravitational wave signals in 2015, resulting from the merger of two stellar black holes, marked the beginning of the era of gravitational wave astronomy. Now, astrophysicists want to write a new chapter and detect gravitational waves in the nanohertz range, which e.g. supermassive black holes orbiting one another create, long before they collide.

Image of OJ 287 taken in the R-band (659nm) with the Schmidt-Teleskop-Kamera at the 0.9-metre reflector at the University Observatory in Großschwabhausen. The one-hour exposure shows several faint galaxies as nebulae located in front of OJ 287, among them the barred spiral galaxy IC 2423 (above). The edge length of the field of view is 18 arcminutes. The picture was taken in the framework of Felix Hildebrandt’s bachelor’s thesis. The physics student at the University of Jena closely studied the current brightness evolution of OJ 287. Image: M. Mugrauer & F. Hildebrandt

An international team of almost 30 research institutions from all over the world has now indirectly detected such a system of supermassive black holes. The scientists have proven that the quasar OJ 287-located approximately four billion light years away in the Cancer constellation-is a binary system of two supermassive black holes whose interaction is believed to lead to the emission of nanohertz gravitational waves. In the current issue of the "Astrophysical Journal Letters" , they present their observational data recorded last year. "The measurements of the Spitzer Space Telescope were assisted by ground based observations", says Dr Markus Mugrauer from the Astrophysical Institute and University Observatory of the Friedrich Schiller University Jena. Both the astrophysicist and Jena physics student Felix Hildebrandt co-authored the current study. They spent many clear nights observing OJ 287 from the University Observatory, located in Großschwabhausen.

The researchers argue that their observations very precisely confirm predictions made based on the general theory of relativity. "We already knew that OJ 287 is a quasar, a quasi-stellar object. It looks like a star through a telescope, but in fact it is the extremely luminous centre of a galaxy far away," explains Mugrauer. What is striking about OJ 287 is the temporal variability of its luminosity: twice in twelve years, the brightness of OJ 287 increases significantly within only two days compared to the rest of the time. Astronomers had attributed this strange behaviour to the theory that there is not only one black hole in the centre of OJ 287, but two supermassive black holes that revolve around each other in an orbital period of twelve years.

Illustration of the relativistic orbit (blue line) of the smaller black hole around the centre of OJ 287 with a larger, more massive black hole (centre of the diagram) that is surrounded by an extensive accretion disk (orange plane at y = 0 AE). It shows the orbit of the companion between 2005 and 2023. The impacts of the companion, which caused OJ 287’s outbursts in 2007 and 2019, occurred at almost the same place in the disk; and the companion had a similar trajectory in both cases, which made the light curves of OJ 287’s outbursts comparable. By contrast, the light curves of the outbursts in 2005 and 2022 are expected to be different. Picture: Laine et al. 2020,Astrophysical Journal Letters, 894, L1

This was only a theory-until a recent observation has provided evidence. Calculations predicted another optical outburst of OJ 287 for the morning of 31 July 2019. "On its orbit, the secondary black hole punches through a gaseous accretion disk that surrounds the primary black hole," explains Mugrauer. Every time this happens, extremely hot gas is released in a big explosion-the outburst that can be observed from the Earth. The outburst calculated to happen in 2019 was predicted to be similar to the one observed in 2007, because the secondary black hole passed through the disk surrounding the primary black hole in almost the same point and direction than 12 years before. And the astrophysicists were able to show exactly that: The telescope registered the expected signal of the outburst in OJ 287’s light curve, with a deviation of less than four hours from the predicted time.

With the help of these observations that are published now, the team of researchers was moreover able to verify a fundamental theorem of black hole physics called "no-hair" theorem. The theorem states that black holes are plain bodies-jokingly "without hair"--, which rules out any unevenness in their event horizons. One way to prove this theorem is to examine a satellite’s movement around a black hole with great precision: If a black hole had edges-"hair"-, then the orbit of the satellite should change in a measurable way. The data recorded now and earlier observations of OJ 287’s outbursts allowed to determine the orbit of the secondary black hole very precisely, which validates the "no hair" theorem.

"The research results we present in our study show the importance of university observatories," Mugrauer summarizes. "Not only do they provide important calibration data for space observation, but they also enable us to continuously observe celestial objects over a very long period of time." In addition, these observatories allow physics students to directly collaborate in international astrophysical research projects.


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