Astronomers using the global radio telescope array have captured a record sharp image of Blazer OJ 287, which shows that its particle jet is bent rapidly. This twisted jet provides compulsive evidence that the OJ 287 core is not one but two super -maternal black holes are included in a tough orbit. For decades, ~ 12 -year -olds of OJ 287 indicated in a secondary black hole, and the new image confirms this model. In fact, it seems that it is the most extreme binary black hole system ever. Researchers say the search makes the OJ 287 an ideal candidate for further research in integrating the gravity waves associated with it.
Twisted jet revealed a cosmic pair
According to the study, using the Earth Space Radio Interfaceometer, astronomers produced a very fast image in the center of the OJ 287. The jet in the picture turns three times faster within ~ 0.3 lights and swings at about 30 ° in a few years. Such a dramatic turning point is naturally described by another black hole at the jet base. It fits the 12-year-old flame of OJ 287: A ~ 150 million-fellow fellow fellow fellow fellow fellow fellow fellow fellow is hollow every 12 years through the primary account disk, leading to bright provocation and turns the jet. Even observations caught a wave of shock in the jet, in which the gamma rays were torn through NASA’s Ferma and Swift satellites. Astronomers say that this divided, ribbon -like jet jet is a clear evidence of two super -maternal black holes locked in the gravity tug of war.
The implications of black hole evolution
The Black Hole for the OJ 287 will eventually be merged, but it will not be a long time. In the meantime, their orbit sends very long wavelengths to gravity waves that the existing detectors cannot lift. Scientists are expected to be Pulse Timing Eri-who monitor the tuck of remote neutrons-this unconscious gravity signal can be detected. Looking forward, future space missions such as ESA/NASA planned Lisa Observatory (2030s) can catch the last integration of such a super -motor couple.
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