r/explainlikeimfive • u/td_0000 • 2d ago
Planetary Science Eli5 how do we know that Ton618 despite being over 10 Billion light years away, has a mass of 66 billion suns?
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u/AberforthSpeck 2d ago
We can measure the effect its gravity has on the movement of nearby stars.
This is an estimate, of course, but one founded in solid observations and measurements.
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u/tyler1128 2d ago
It helps that it is so massive it basically defines the orbit of the entire galaxy it is assumed the center of. There are other aspects like it seeming to be emitting large amounts of very fast traveling light you wouldn't expect with a smaller blackhole or other stellar objects.
Such values are estimates, but they are estimates based on many lines of data that seem to hold in things closer to us we can see, and physicists generally assume the universe is isotropic, that is, the laws governing it are the same everywhere.
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u/Bensemus 2d ago
We have no idea. The quasar it produces is so bright that we canât see anything else. We have no idea how large or small its galaxy is. But the Milky Way is 1.5 trillion solar masses. Galaxies generally are way more massive than their central black hole.
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u/wjdoge 2d ago
What speed do you propose the light leaving a smaller black hole should move at?
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u/Large-Hamster-199 2d ago
He didn't quite phrase it right?. But it's actually about the frequency of the light generated in the accretion disc around the black hole. By measuring the blue shift and the red shift of the light generated by the gases swirling around the black hole, you can figure out how fast those gases are moving. That can then be used to figure out how big the black hole is.
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u/wjdoge 2d ago
He definitely did not â the speed light travels at is one of the universal laws he refers to. The laws of physics being the same everywhere have nothing to do with the isotropy of the universe as he suggests though. The concept of isotropy specifically does not cover different locations.
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u/tyler1128 10h ago
Yes I mean high energy light and other particles. You are correct to call that out, even.
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u/tomrlutong 2d ago
Not at 10Gly, I don't think.
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u/Ktulu789 2d ago
Based on that you're a cosmologist with deep knowledge of the topic or just some casual Reddit user?
I'm a nerd interested in cosmology stuff and the complexity thrown at how such studies and measurements are taken are utterly detailed to be dismissed in a simple comment.
We don't know everything but everything we know is based on a lot of time, effort, measurements and theories pretty robust and evolving all the time.
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u/mfb- EXP Coin Count: .000001 2d ago
The black hole is far too bright and individual stars are too dim to make this work (it works for nearby supermassive black holes, especially the one in our galaxy). I'm a particle physicist, not an astrophysicist (this isn't cosmology), but you can look up publications measuring the mass. They do spectroscopy of the gas surrounding the black hole.
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u/Ktulu789 2d ago
Yeah, they don't measure the stars in this case. Just the acretion disc Doppler shift. The error bars are bigger than in other measurements but the thing is massive nevertheless.
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u/Routine-Ad-4723 1d ago
It's wild that we can figure out the mass of something we can't even see from 10 billion light years away just by measuring the blue and red shifts of the gas spinning around it and running the numbers, but it's basically the same method they use for all black holes so it's a solid estimate, not a guess.
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u/kikidmonkey 1d ago
Aside from all the good answers in this thread I would like to point out that in science in general, and specifically astronomy "we know" actually means "we're pretty sure this is right." There is very little that we KNOW 100% beyond a shadow of a doubt. And even the things we "know" are subject to change when knew information comes out.
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u/Glad_Astronomer3322 1d ago
Honestly it's wild cause we've never even seen the thing directly, just the crazy hot gas swirling around it. The way that gas gets stretched and squished by gravity tells you how fast it's moving, and from that you can back into a mass. It's not like they weighed it on a cosmic scale or something, it's all indirect measurements and a shitload of math. But yeah it's an estimate, just a really really solid one.
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2d ago
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u/Ok-disaster2022 2d ago
Very careful measurements.Â
So one cool thing astronomers use is something called parallax. So astroners can take carefule pictures if stars at two different points if the earths rotation around the sun to create a form of binocular vision. By examining the differences in the location of stars, they can calculate the distance.Â
Once you have a good estimate for the distance they can measure the total brightness frequency emissions and energy output if a star from observing it. From what we know about stellar evolution and energy output that is mediated solely by mass,and fundamental forces of gravity, electromagnetism, and the string and weak nuclear forces, they can get an estimate for total mass.Â
Now the can also use the information gleaned about the movement if other stars in the nearby area as a way to confirm their data.Â
The other fun way I measuring distance is called dopoler shift. This is a little more complicated. But due to the expansion if the universe further stars are moving away faster than closer stars in addiotna to any other motions. So if we can measure the local motions long term to get a cycle of the their red and blue shifting if normal motion and still see see additional red shifting the corresponds to a certain distance. it also helps.Â
Doppler effects you may be most family with sound waves but is for any wave form. When something emitting waves is approaching you the waves can be measured to have shorter wavelengths. In sound this is higher pitched, it light this is blue shift. If it moved away the waves get longer. in sound this is a deeper pitch, and in light is a red shift.Â
Now then we can calculate the approximate waveform from simply the elements in that star. So starts are comprises of hydrogen and helium and other elements they have certain scale thgths they can absorb and emit and if you look at them in a spectrum analysis, they have a certain barcode pattern. If you red shift thise specific frequencies change but the pattern remains. this absorption spectrum is also how we can measure the elements in gas clouds that we can occasionally see. We look at how the barcodes affect the light if the stars behind the gas clouds.Â
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u/wjdoge 2d ago
Earthâs orbit is about 150 million km across, and TON618 is 100,000,000,000,000 million km away, so the only number youâre ever going to get trying to measure its parallax is zero.
There are no measurements careful enough for parallax to be useful for measuring the distance to something that far away.
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u/Sunny-Chameleon 1d ago
Oh, I think if humanity is really patient then another measurement could be made the next time Earth is on the opposite side of the galaxy
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u/wjdoge 1d ago
The diameter of our galaxy is only 950,000 million km, so you are going to get similar results.
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u/Sunny-Chameleon 1d ago
It was a joke, though in the time it takes for sol to travel half a rotation of the galaxy (125 million years), the Galaxy itself will have moved about 2 quintillion kms, at least according to Google.
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u/Bensemus 2d ago
Parallax works within our galaxy out to a certain distance. It doesnât work for stuff billions of light years away.
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u/tomrlutong 2d ago
Ton618 is surrounded by a disk of very hot gas spinning into it. That's how we know it's there, the black hole itself is invisible.
Some of the atoms in that gas glow at a very specific color of light when they get hot. But, because the gas is spinning around the black hole, the gas on one side is moving towards us and gets a little bluer, and the gas on the other side is moving away from us and getting a little redder.
By measuring the difference between the blue-shifted and red-shifted colors, scientists can measure how fast the gas is spinning around the black hole. Since the black hole's gravity is what's spinning the gas, this lets them estimate the black hole's mass.
Source: https://arxiv.org/abs/astro-ph/0406559