One more flare happened since then, in 2022, but because of instrumental limitations, it was caught only at a prestage (M. J. Valtonen et al. 2023; M. J. Valtonen 2024). At the same time, more flares were discovered in historical photographic plate studies so that only eight of the expected 26 flares remain unconfirmed (R. Hudec et al. 2013). All the unconfirmed ones are due to lack of known photographs at the expected epochs.
When two galaxies merge, their supermassive black holes fairly rapidly sink to the center of mass of the newly combined galaxy via dynamical friction and enter into a slow orbit around each other. Over time, the SMBHs kick out interloping stars, which removes energy from the orbit and causes the two SMBHs to come closer together. If the SMBHs were able to get within ~0.1 parsecs of each other, gravitational wave radiation could take over and cause the orbit to shrink fairly rapidly and lead to the merger of the two SMBHs.
However, the theoretical models we have generally predict that at about 1 parsec, the SMBHs have kicked out all the stars in their neighborhood, so the process stalls out. In practice we don't observe many SMBH binary systems (OJ287 being the main exception), so there must be some mechanism that causes these systems to shrink from 1 pc to 0.1 pc. But we don't know what it is. The hope is that detailed studies of the orbit of OJ287 can provide some clues as to what that missing mechanism is.
pavel_lishin•1h ago
Damn, that's about the time it takes Jupiter to orbit the sun. That feels wildly close together for objects that mass 18 billion & 150 million times that of our own sun.
These black holes (according to a calculator I found online) have radii of 53 billion km and 400 million km, so I'm guessing they must be orbiting significantly further away, and significantly faster than Jupiter (which is ~800 million km away from the sun) - which makes sense, given the monstrous 18b figure. I wonder how far apart they are, but I don't really know how to easily calculate that right now.
hinkley•1h ago
I’m having more trouble visualizing how accretion disks would work for a binary black hole. Because the light is coming from the disks, not the black holes. So those are what are actually pulsing/girating.
pavel_lishin•1h ago
I thought that in this case, the light that they detected was coming from the jets coming from the poles, not the disk itself directly.
hinkley•1h ago
ardel95•1h ago
ardel95•1h ago
kmm•1h ago
Plugging 12 years and 18e9 solar masses gives about 2e12 kilometers, or roughly a fifth of a lightyear. This also means the smaller black hole is zipping around the bigger one at around 6% of the speed of light, which is low enough that the Newtonian approximation is probably reasonable accurate (at least to give a rough idea of how large the distances must be).
hnuser123456•1h ago
[1] https://archive.is/Ccy5M
edit: just noticed the issue with 502,000 km/s being more than c... recalculating before I can't edit!
edit2: this is gemini's 2nd attempt, and seems more realistic, sorry don't have time to deep dive to verify...
IAmBroom•30m ago
ccozan•17m ago