<p>I once heard of a Japanese cartoon/movie/show where space pirates threatened to compress the planet Jupiter into a black hole and thus destroy half the Milky Way galaxy.</p>

<p>It sounds like an interesting idea, but... even if you could compress Jupiter into a black hole, its mass would remain the same, meaning that Jupiter (now a black hole) would still continue to move around our sun in its same orbit, and Jupiter's moons would still continue to orbit Jupiter as they did before.</p>

<p>Many people think that once a star collapses into a black hole, its "sucking power" (its gravitational force) increases.  This is simply not the case.  Believe it or not, many stars are <em>less</em> massive <em>after</em> they turn into a black hole than <em>before</em>, when they were shining stars.  This is because, at the end of their lives, some stars shed a significant portion of their outer layer into space right before they collapse into a black hole.</p>

<p>I've read that if you compressed the Earth to the size of a cherry, its density would be so great that it would turn into a black hole.  Assuming that were true and it was actually done, the black hole of Earth would still continue orbiting the sun once every year, and Earth's moon would continue to orbit the Earth about once every 29.5 days.  (Now, the spin of the new black-hole-Earth about its axis would probably be different, but the time it would take to orbit the sun would not change.)</p>

<p>Surprisingly, once the Earth got compressed into a cherry-sized black hole, less space debris would fall into it than before (when the Earth was the size of... well, Earth).  This is because the newly-formed black-hole-Earth would take up much less space (volume) and asteroids and comets would be more likely to miss the cherry-sized (or slightly-larger-than-cherry-sized) volume that, if not missed, would cause the debris to be sucked into the black hole.</p>

<p>If the debris missed the black-hole-Earth by even a kilometer (which might seem like a large distance to us, but is very miniscule in astronomical terms), it would be flung off in a different direction, possibly never to return.</p>

<p>So, basically, a common misconception people have regarding black holes is that nothing has more gravity than a black hole, and that stars that form into black holes all of a sudden have increased gravity and therefore get more "sucking power."  This is simply not true.  Black holes still have the same mass as before (sometimes less, depending on how they're formed), and how much "sucking power" they have is still dependent on how much mass they're made up of.</p>

<p>While it may be true that the most massive stars in the universe are indeed black holes (if you'd even call them <em>stars</em> at that point), there exist many stars that are more massive (and therefore have more "sucking power") than many black holes.</p>

<p>So the fact that our galaxy's center probably contains a super-massive black hole doesn't mean that the black hole would suck up any more matter than if it were the same amount of mass which happened to not be in black-hole-form.</p>

CC BY-SA 3.0
2017-12-22T22:41:00.877Z
Another inaccuracy about space pirates destroying half the Milky Way with a black hole is the fact that any changes in Jupiter's gravitational field would not propagate faster than light and thus would take tens of thousands of years for all this destruction to be finished.
Michael
CC BY-SA 3.0
2017-12-23T21:38:36.440Z
Also, isn’t destroying the galaxy sort of counter to the usual aims of piracy?
rickster
CC BY-SA 3.0
2017-12-24T00:18:16.810Z
Nice and clear reminder of a common misconception. Thanks for pointing out that a black hole is no less no more than a gravitational object.
Benj
CC BY-SA 3.0
2017-12-21T19:53:37.543Z
2017-12-22T08:54:27.920Z
2017-12-22T08:54:27.920Z
J-L
<p>Gravity follows the law of inverse square.  To put it simply if you double the distance from a gravity source you quarter is effect.  So if you double the distance you are from the earth you feel 1/4g. It's important to note that as the distance increases it will never be 0, it will always be some non-zero value no matter the distance.</p>

<p>So at galactic distances the force of gravity the central black hole has very little effect. </p>

<p>This only explains part of it.  The other part is conservation of angular momentum.</p>

<p>The force of gravity and the angular momentum is what is responsible for orbits.  In orbital mechanics you raise your orbit by adding speed, not altitude.  Your adding angular momentum which raises your orbit.  To lower your orbit you reduce you speed which reduces your angular momentum and your altitude.</p>

<p>So for things to "fall" into a black hole they must be travailing at a speed where their orbit intersects the event horizon. This is rarely the case or those "things" wouldn't truly be in orbit to begin with. So the very fact that all the "stuff" that makes up the galaxy orbits the central black hole means that it cant just fall into it.</p>

<p>These 3 things are always in balance in a stable orbit, force of gravity, speed and altitude ( or distance from the gravity source ).  If you change one of them the other 2 must also changes.  If you decrease speed your altitude goes down, and the gravity increases.  If you increase the gravity the speed must also increase or the altitude will decrease.</p>

<p>So you see things can't just fall into the black hole.  That said it is my view that eventually everything in the galaxy will fall into the central black hole, however this will take many billions of years.</p>

<p>Of course this is overly simplifying things, and I am by no means an expert on this stuff.  But it's something I can picture in my mind, the balance between momentum and gravity.</p>

<p>v</p>

CC BY-SA 3.0
2017-12-25T04:08:17.477Z
2018-01-08T18:56:51.650Z
2018-01-08T18:56:51.650Z
ArtisticPhoenix
<p>You must also factor in the dark matter which is interacting gravitationally with all of the "hot matter" that can be seen in the galactic disk. Dark matter was  discovered by carefully mapping the orbits of objects in galaxies and finding that the matter that could be seen could not account for the observed orbital motion. One of the mysteries of dark matter is that it is not pulled into the black hole the way hot matter is. The dark matter has the practical effect of balancing out some of the gravitational pull of the supermassive black hole at the galaxy's center. </p>

CC BY-SA 3.0
2017-12-21T07:31:24.807Z
It depends on how the matter is distributed. Dark matter is generally thought to occur in a sphere around the galaxy. For a spherical distribution of matter, you only need to concern yourself with the portion interior to your orbit; what's outside won't affect you. So dark matter will still have the same result of pulling you inwards.
Phiteros
CC BY-SA 3.0
2017-12-20T20:53:30.697Z
2017-12-20T20:53:30.697Z
Steven Liszewski
<p>Well, I'm not a physics student, but I think people usually nurture the misconception of "sucking power" of a black hole for a reason. </p>

<p>Let us consider Newton's equation for gravity:</p>

<p>$F = {Gm_im_j\over r_{ij}^2}$
for two bodies i and j, and $r_{ij}$ is the distance between the centre of mass of two bodies.</p>

<p>Now, if the Sun today suddenly decided to become a black hole without shedding weight, it won't affect Earth's orbit, because even if Sun's volume has changed, $r_{ij}$ remains constant.</p>

<p>The reason why Black Holes "suck" is because, since they occupy extremely less volume compared to planets and stars, you can get the $r_{ij}$ component to be really really small.</p>

<p>Correct me if I'm wrong.</p>

CC BY-SA 3.0
2017-12-25T16:32:58.660Z
2017-12-25T16:32:58.660Z
Sabyasachi Mukherjee
<p>For galaxies with large black holes, the surrounding matter is in <em>orbit</em> around the black hole(s), the same way that the moon orbits the earth.</p>

<p>The question is a direct analogy to "<em>Why doesn't the Moon fall to the ground?</em>" or "<em>Why don't the planets fall into the sun?</em>".  The black hole is more massive than the Sun, but its effects are of the same type.</p>

CC BY-SA 3.0
2017-12-21T19:30:32.930Z
That is not a typical situation at all. In the vast majority of cases the black hole is a tiny fraction of the total mass of the galaxy. There are some outliers, sure, but they are the exceptions.
Florin Andrei
CC BY-SA 3.0
2017-12-22T08:56:00.803Z
Perhaps it's fairer to say that the black holes and other matter are all in orbits with each other.  Anyway, the important point is that there's a good analogy with the question most of us asked as children.
Toby Speight
CC BY-SA 3.0
2017-12-22T19:10:00.213Z
I'm sorry, but it's not a good analogy. What you're describing is literally a handful of cases out of countless millions.
Florin Andrei
CC BY-SA 3.0
2017-12-21T17:09:49.977Z
2017-12-21T17:09:49.977Z
Toby Speight
<p>One quick answer for your question would be event horizon or Schwarzschild radius. Anything which is fairly close to this radius/horizon will eventually be sucked up by the black hole.  </p>

CC BY-SA 3.0
2017-12-21T19:00:03.677Z
2017-12-21T19:00:03.677Z
user1157
<p>The simple answer is that everything else in the galaxy is going sideways fast enough to escape being sucked in. Instead, the force of the suck (if you like) causes the stars' paths to be pulled into a circle around the black hole.</p>

<p>This phenomenon is "orbit". As other answers pointed out, it's the same reason the Earth does not fall into the Sun, or the Moon fall onto the Earth, and why the International Space Station is hurtling along at around 17,150 miles per hour. They're all going sideways, the force of some large object is turning that sideways motion into circular motion, and if they weren't going fast enough then they'd curve ("fall") towards that large object and crash into it.</p>

<p>It's like if you whirl a bucket on the end of a string. The bucket is going sideways, but the string is pulling it towards you. The bucket doesn't fly off away from you because of the force from the string, and so it curves in a circle. The force from the string happens to not be enough to collapse the bucket inwards and hit you.</p>

CC BY-SA 3.0
2017-12-22T01:15:17.757Z
2017-12-22T01:15:17.757Z
Len has moved to Codidact
<p>Be patient, eventually it will unless the galaxy's rate of expansion exceeds the black hole's gravitational growth as it consumes the matter around it.</p>

<p>In that scenario the galaxy will eventually diffuse, with its matter continuing to travel away from the black hole until it encounters another galaxy, at which point it stands a good chance of eventually getting sucked into that's galaxy's black hole. Nothing survives forever.. :-) </p>

CC BY-SA 3.0
2018-01-09T00:18:27.547Z
What makes you think that the galaxy is expanding? Sure, the universe is expanding, but that's only happening on the very large scale. Individual galaxies and even galaxy clusters aren't expanding because their gravity is stronger than the expansion at that scale.
PM 2Ring
CC BY-SA 3.0
2017-12-25T16:39:36.760Z
2017-12-25T16:39:36.760Z
Dan
<p>This is a common misconception about black holes: that they somehow 'suck up' everything around them or pull things into them.  In reality you could replace the Sun now with a black hole of the same mass and not notice any immediate difference.  It's not like it would suddenly start hoovering in the planets around it, that's just not how it works.</p>

CC BY-SA 3.0
2017-12-22T12:31:55.290Z
2017-12-22T12:31:55.290Z
Hollis Williams
<p>its all about ENTROPY which is proportional to the surface area of the event horizon of a black hole(see below for a heuristic quantum  argument due to Moffat/Wang as to why this is so).</p>

<p>Assuming a Schwarzschild  solution gives a radius of 2Gm for the event horizon with m the black hole mass and G Newton's constant. Adding mass to a black hole thus increases its entropy. Given an isolated system of finite total energy, it has a finite maximum entropy which acts as an attractor for the dynamics of the system,placing a limit on the horizon.</p>

<p>J von Neumann defines a quantum version of entropy as follows: Let f be a normal state of a local algebra of observables O(D) acting on the Hilbert space H. Then we can write this f as a convex sum of pure states. For a system of finite energy this sum is finite since H is then finite dimensional
Von Neumann’s non-commutative equivalent of a partition is the density operator   ie the weighted sum of the projections  onto the minimal vector spaces corresponding to these pure states
    Then we have the well-known equivalence;<br>
For such a normal state f, the von Neumann entropy is defined as  the entropy of the weights . We interpret it as an (inverse) measure of the amount of information that the quantum system in a given state will yield through measurement. The larger the entropy of the quantum system, the less information can be extracted. 
<strong>The von Neumann Entropy of a Black Hole</strong>
The measurement process cannot be performed by an external observer to elements within the interior, beyond the event horizon. We thus partition the event horizon of the black hole with elements each of area   k squared, where k is the Planck length and assume the Planck area  corresponds classically to the minimal projection   of the pure vector state  . Let N be the total finite number of partitions. By the ‘no hair’ hypothesis there is no preferred location on the event horizon, so that each partition element must have the same weighting. The von Neumann entropy of this partition is thus proportional to S the surface area of the black hole.</p>

CC BY-SA 3.0
2017-12-21T19:17:45.133Z
While black hole entropy and the Beckenstein bound is an important and fascinating topic, I fail to see how it's particularly relevant to the OP's question.
PM 2Ring
CC BY-SA 3.0
2017-12-22T09:35:51.340Z
This is a copypasta of https://www.researchgate.net/profile/Charles_Wang28/publication/313904636_Additional_Online_Material_For_%27Quantum_Ergodic_Theory_and_Diffeomorphism_Invariant_Quantum_States%27/data/58af52feaca2725b5411233c/additional-online-material-for-quantum-ergodic-theory.pdf with no relevance to the OP's question.
MBR
CC BY-SA 3.0
2017-12-22T14:08:23.767Z
I improved my answer to take account of the kind comments
Prof James Moffat
CC BY-SA 3.0
2017-12-21T16:44:16.387Z
2017-12-22T14:06:48.020Z
2017-12-22T14:06:48.020Z
Prof James Moffat
<p>You shouldn't think of black holes as "sucking things in". Black holes interact with matter through gravity, just the same as any other object. Think of our Solar System. All the planets orbit around the sun because it has a lot of mass. Since the planets have some lateral motion (they're not moving directly towards or away from the sun), they circle around it. This is known as <a href="https://en.wikipedia.org/wiki/Angular_momentum#Conservation_of_angular_momentum" rel="noreferrer">conservation of angular momentum</a>.</p>

<p>When talking about gravity, all that matters is the mass of the objects involved. It doesn't really matter what kind of object it is*. If you were to replace the sun with a black hole that had the same mass as our sun, the planets would continue on the exact same orbits as before.</p>

<p>Now, the black holes at the centers of most spiral galaxies do accumulate mass. Some of these black holes have <a href="https://en.wikipedia.org/wiki/Accretion_disk" rel="noreferrer">accretion disks</a> around them. These are swirling disks of gas and dust that is slowly falling into the black hole. These gas and dust particles lose their angular momentum through interactions with gas and dust nearby and by radiating energy as heat. Some of these black holes have very large accretion disks, and can generate huge amounts of electromagnetic radiation. These are known as <a href="https://en.wikipedia.org/wiki/Accretion_disk" rel="noreferrer">active galactic nuclei</a>.</p>

<p>So, long story short, black holes don't "suck". They just interact with things gravitationally. Stars, gas, and other matter in the galaxy has angular momentum, so it stays in orbit around the center of the galaxy. It doesn't just fall straight in. This is the same reason the Earth orbits around the Sun. </p>

<p>*Disclaimer: When you talk about things like tidal forces, you do need to take into account the size of the objects. But for orbital mechanics, we don't need to worry about it because the distances between the objects are generally much larger than the objects themselves.</p>

CC BY-SA 3.0
2017-12-19T22:59:07.823Z
To add, if the Sun became a black hole, and if it managed to do so without losing mass, Earth and the rest of the solar system will continue to orbit around it as they always have. You only end up getting "sucked into" the black hole if you get really close to it, at which point the gravitational force is tremendous. But you have to get really close. For illustration, the Earth would need to be compressed to ~1 cm wide to become a black hole. In real life, even if you tunnel to the Earth's core, you won't feel that kind of gravity since the mass is above you (see the shell theorem).
Allure
CC BY-SA 3.0
2017-12-20T00:00:00.683Z
"Some of these galaxies have very large accretion disks" I think you meant "Some of these *black holes*..."
jpmc26
CC BY-SA 3.0
2017-12-20T00:45:11.713Z
@jpmc26 Indeed I did, thanks for the catch.
Phiteros
CC BY-SA 3.0
2017-12-20T02:34:43.040Z
Possible pedantic caveat - on a long enough timescale one might expect the various objects orbiting a galactic black hole to eventually fall into it as friction with the interstellar medium gradually depletes their angular momentum.  Of course, the density of the interstellar medium is so low that "a long enough timescale" is probably absurdly, ridiculously long (almost certainly longer than the lifespan of any object in the galaxy).
aroth
CC BY-SA 3.0
2017-12-20T05:50:08.597Z
@aroth Yes, I was considering adding some more footnotes about how things lose angular momentum and the fact that the galaxy isn't orbiting around the black hole per se, but about the center of mass of the entire galaxy. But adding too much detail can cause confusion. Generally I find that it's best to answer the question simply without adding too much extra information. If they want to find out more about a particular aspect, they can ask another question.
Phiteros
CC BY-SA 3.0
2017-12-20T08:21:53.763Z
Thanks a lot, now I understood. So if an object is not too close to the black hole so that the last one exerts a very strong gravitational force nothing happens.
OiRc
CC BY-SA 3.0
2017-12-20T13:27:17.790Z
I have just realized that a galaxy is essentially just a giant accretion disk for the supermassive black hole in the middle...
John Dvorak
CC BY-SA 3.0
2017-12-20T16:03:03.680Z
@OiRc That's essentially correct. Black holes aren't a cosmic vacuum cleaner, they're just a really massive celestial object that exerts gravitational force the same way as anything else does. Until you get close enough to start breaking General Relativity (ie: crossing the event horizon), you can think of them working the same as a really big star (because that's basically what they are, the star just died).
thanby
CC BY-SA 3.0
2017-12-20T16:10:19.890Z
@JohnDvorak Bingo. And the reverse is also true; Planets/asteroids are just the accretion disc of their respective star(s), moons are the accretion disc of planets... Everything started from big clouds of dust that slowly clumped up into bigger and bigger objects. (That's a bit simplified, but generally accurate.)
thanby
CC BY-SA 3.0
2017-12-21T00:09:24.190Z
@JohnDvorak Not the same thing at all. The black hole + accretion disk system is vastly dominated and is driven by the gravity of the black hole. Big as the supermassive black hole may be, it's just a speck of dust at the scale of the whole galaxy. The galaxy is a very different system from an accretion disk - it's held together by its own total gravity, as opposed to merely orbiting a black hole.
Florin Andrei
CC BY-SA 3.0
2017-12-21T13:25:07.177Z
If planets can orbits black holes , then can black hole act as source of energy like our sun ? if so then can these planets habitable ?
Rahul Rabhadiya
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2017-12-21T17:53:06.463Z
I think this is where we go "Any sufficiently granular accretion disk is indistinguishable from orbiting bodies." lol
Kaithar
CC BY-SA 3.0
2017-12-21T18:12:48.813Z
@RahulRabhadiya Yes and no, but practically speaking far more no than yes. Ultimately, the sun is an energy source because it radiates colossal amounts of electromagnetic radiation (light), not because of its gravity. Black holes are literally defined by having gravity so strong that light cannot escape, which means they do not radiate light in the same way. That’s the big no: the sun’s gravity is not why it is a good energy source, and the black hole’s gravity actually makes it a *bad* energy source.
KRyan
CC BY-SA 3.0
2017-12-21T18:20:08.283Z
@RahulRabhadiya On the other hand, there is a kind-of yes to your question. Black holes are hypothesized to emit “Hawking radiation,” which is also electromagnetic radiation (light). That’s complicated, but for a black hole the mass of the sun, its effective temperature would be 60 billion*ths* of a degree above absolute zero. It would absorb more energy from the cosmic background radiation than it emits, so it would be a net reduction in energy. Hawking radiation goes *down* with larger black holes, too, so to get more energy you need smaller black holes—which need smaller things orbiting.
KRyan
CC BY-SA 3.0
2017-12-21T20:41:50.560Z
"Now, the black holes at the centers of most spiral galaxies do accumulate mass".  Doesn't that mass *growth* change the surrounding orbits?  Or is that growth insignificant when compared to the mass of the black hole?
Nathan Merrill
CC BY-SA 3.0
2017-12-24T23:08:15.847Z
One could add that anything that *didn't* have sufficient angular momentum, i.e. was on a collision course, has fallen in long ago. What has survived had the properties necessary to survive. The cosmos, as anything else, is subject to the basic principles of evolution; that which is not sustainable tends to disappear (which is somewhat tautological, it's that basic).
Peter - Reinstate Monica
CC BY-SA 3.0
2017-12-26T14:43:56.973Z
@NathanMerrill: The mass they're consuming was already there. No mass is created or destroyed when the black hole absorbs it. From the perspective of anything orbiting any meaningful distance away, the difference between "mass near the black hole" and "mass consumed by the black hole" is irrelevant.
ShadowRanger
CC BY-SA 3.0
2017-12-19T19:01:18.163Z
2017-12-20T00:45:24.557Z
2017-12-20T00:45:24.557Z
Phiteros
<p>As stated in several sources, it's supposed that in every galaxy there is a black hole in the middle.</p>

<p>My question is, <em>why do these black holes in the middle of galaxies not suck up all the surrounding matter in the galaxy?</em></p>

CC BY-SA 3.0
2017-12-20T14:34:23.203Z
Obligatory [xkcd](https://what-if.xkcd.com/58/).
Raidri
CC BY-SA 3.0
2017-12-20T15:49:12.277Z
@Raidri There's also a good one about the relationship between mass and gravity in the *What-If* book. IIRC it discusses what effects a chunk of "neutron star material" would do locally on earth. Long story short: Don't touch it. If you haven't already, I highly suggest picking up a copy (of the book, not the neutron star).
thanby
CC BY-SA 3.0
2017-12-21T13:20:56.257Z
Please don't use the comment space for answers.
called2voyage
CC BY-SA 3.0
2017-12-21T15:47:19.403Z
Similar: 

https://astronomy.stackexchange.com/questions/21443/what-is-this-bright-glow-in-the-center-of-galaxies
K Split X
CC BY-SA 3.0
2017-12-21T22:46:21.063Z
Last I knew, it was not supposed that "in ***every*** galaxy there is a black hole in the middle." Notice the emphasis on *every*. Should edit "every galaxy" to "many galaxies"
Aaron
CC BY-SA 3.0
2017-12-22T00:01:05.777Z
Matter in a galaxy are spread VERY far apart. A SMBH wouldn’t have the gravitational force to “suck” it all up.
NuWin
CC BY-SA 3.0
2017-12-23T19:18:02.650Z
@Raidri Also relevant (especially the 3rd paragraph): https://what-if.xkcd.com/129/
NobodyNada
CC BY-SA 3.0
2017-12-25T00:46:17.530Z
For the same reason that the star at the centre of the solar system doesn't suck up all the planets.
David Richerby
<black-hole><galaxy>
Why do Black Holes in the middle of galaxies not suck up the whole galaxy?
OiRc
# Why do Black Holes in the middle of galaxies not suck up the whole galaxy?

(Asked by: username_0 on 2017-12-19)

As stated in several sources, it's supposed that in every galaxy there is a black hole in the middle.

My question is, *why do these black holes in the middle of galaxies not suck up all the surrounding matter in the galaxy?*

**Tags:** black-hole, galaxy

> **Comments:**
> **username_1**: Obligatory [xkcd](https://what-if.xkcd.com/58/).  
> **username_2**: @username_1 There's also a good one about the relationship between mass and gravity in the *What-If* book. IIRC it discusses what effects a chunk of "neutron star material" would do locally on earth. Long story short: Don't touch it. If you haven't already, I highly suggest picking up a copy (of the book, not the neutron star).  
> **username_3**: Please don't use the comment space for answers.  
> **username_4**: Similar:   https://astronomy.stackexchange.com/questions/21443/what-is-this-bright-glow-in-the-center-of-galaxies  
> **username_5**: Last I knew, it was not supposed that "in ***every*** galaxy there is a black hole in the middle." Notice the emphasis on *every*. Should edit "every galaxy" to "many galaxies"  
> **username_6**: Matter in a galaxy are spread VERY far apart. A SMBH wouldn’t have the gravitational force to “suck” it all up.  
> **username_7**: @username_1 Also relevant (especially the 3rd paragraph): https://what-if.xkcd.com/129/  
> **username_8**: For the same reason that the star at the centre of the solar system doesn't suck up all the planets.  

---

## 11 answers

### Answer by username_15 on 2017-12-19. Score: 87 | Accepted answer

You shouldn't think of black holes as "sucking things in". Black holes interact with matter through gravity, just the same as any other object. Think of our Solar System. All the planets orbit around the sun because it has a lot of mass. Since the planets have some lateral motion (they're not moving directly towards or away from the sun), they circle around it. This is known as [conservation of angular momentum](https://en.wikipedia.org/wiki/Angular_momentum#Conservation_of_angular_momentum).

When talking about gravity, all that matters is the mass of the objects involved. It doesn't really matter what kind of object it is\*. If you were to replace the sun with a black hole that had the same mass as our sun, the planets would continue on the exact same orbits as before.

Now, the black holes at the centers of most spiral galaxies do accumulate mass. Some of these black holes have [accretion disks](https://en.wikipedia.org/wiki/Accretion_disk) around them. These are swirling disks of gas and dust that is slowly falling into the black hole. These gas and dust particles lose their angular momentum through interactions with gas and dust nearby and by radiating energy as heat. Some of these black holes have very large accretion disks, and can generate huge amounts of electromagnetic radiation. These are known as [active galactic nuclei](https://en.wikipedia.org/wiki/Accretion_disk).

So, long story short, black holes don't "suck". They just interact with things gravitationally. Stars, gas, and other matter in the galaxy has angular momentum, so it stays in orbit around the center of the galaxy. It doesn't just fall straight in. This is the same reason the Earth orbits around the Sun.

\*Disclaimer: When you talk about things like tidal forces, you do need to take into account the size of the objects. But for orbital mechanics, we don't need to worry about it because the distances between the objects are generally much larger than the objects themselves.

> **Comments:**
> **username_26**: To add, if the Sun became a black hole, and if it managed to do so without losing mass, Earth and the rest of the solar system will continue to orbit around it as they always have. You only end up getting "sucked into" the black hole if you get really close to it, at which point the gravitational force is tremendous. But you have to get really close. For illustration, the Earth would need to be compressed to ~1 cm wide to become a black hole. In real life, even if you tunnel to the Earth's core, you won't feel that kind of gravity since the mass is above you (see the shell theorem).  
> **username_27**: "Some of these galaxies have very large accretion disks" I think you meant "Some of these *black holes*..."  
> **username_15**: @username_27 Indeed I did, thanks for the catch.  
> **username_28**: Possible pedantic caveat - on a long enough timescale one might expect the various objects orbiting a galactic black hole to eventually fall into it as friction with the interstellar medium gradually depletes their angular momentum.  Of course, the density of the interstellar medium is so low that "a long enough timescale" is probably absurdly, ridiculously long (almost certainly longer than the lifespan of any object in the galaxy).  
> **username_15**: @username_28 Yes, I was considering adding some more footnotes about how things lose angular momentum and the fact that the galaxy isn't orbiting around the black hole per se, but about the center of mass of the entire galaxy. But adding too much detail can cause confusion. Generally I find that it's best to answer the question simply without adding too much extra information. If they want to find out more about a particular aspect, they can ask another question.  
> **username_0**: Thanks a lot, now I understood. So if an object is not too close to the black hole so that the last one exerts a very strong gravitational force nothing happens.  
> **username_29**: I have just realized that a galaxy is essentially just a giant accretion disk for the supermassive black hole in the middle...  
> **username_2**: @username_0 That's essentially correct. Black holes aren't a cosmic vacuum cleaner, they're just a really massive celestial object that exerts gravitational force the same way as anything else does. Until you get close enough to start breaking General Relativity (ie: crossing the event horizon), you can think of them working the same as a really big star (because that's basically what they are, the star just died).  
> **username_2**: @username_29 Bingo. And the reverse is also true; Planets/asteroids are just the accretion disc of their respective star(s), moons are the accretion disc of planets... Everything started from big clouds of dust that slowly clumped up into bigger and bigger objects. (That's a bit simplified, but generally accurate.)  
> **username_18**: @username_29 Not the same thing at all. The black hole + accretion disk system is vastly dominated and is driven by the gravity of the black hole. Big as the supermassive black hole may be, it's just a speck of dust at the scale of the whole galaxy. The galaxy is a very different system from an accretion disk - it's held together by its own total gravity, as opposed to merely orbiting a black hole.  
> **username_30**: If planets can orbits black holes , then can black hole act as source of energy like our sun ? if so then can these planets habitable ?  
> **username_31**: I think this is where we go "Any sufficiently granular accretion disk is indistinguishable from orbiting bodies." lol  
> **username_32**: @username_30 Yes and no, but practically speaking far more no than yes. Ultimately, the sun is an energy source because it radiates colossal amounts of electromagnetic radiation (light), not because of its gravity. Black holes are literally defined by having gravity so strong that light cannot escape, which means they do not radiate light in the same way. That’s the big no: the sun’s gravity is not why it is a good energy source, and the black hole’s gravity actually makes it a *bad* energy source.  
> **username_32**: @username_30 On the other hand, there is a kind-of yes to your question. Black holes are hypothesized to emit “Hawking radiation,” which is also electromagnetic radiation (light). That’s complicated, but for a black hole the mass of the sun, its effective temperature would be 60 billion*ths* of a degree above absolute zero. It would absorb more energy from the cosmic background radiation than it emits, so it would be a net reduction in energy. Hawking radiation goes *down* with larger black holes, too, so to get more energy you need smaller black holes—which need smaller things orbiting.  
> **username_33**: "Now, the black holes at the centers of most spiral galaxies do accumulate mass".  Doesn't that mass *growth* change the surrounding orbits?  Or is that growth insignificant when compared to the mass of the black hole?  
> **username_34**: One could add that anything that *didn't* have sufficient angular momentum, i.e. was on a collision course, has fallen in long ago. What has survived had the properties necessary to survive. The cosmos, as anything else, is subject to the basic principles of evolution; that which is not sustainable tends to disappear (which is somewhat tautological, it's that basic).  
> **username_35**: @username_33: The mass they're consuming was already there. No mass is created or destroyed when the black hole absorbs it. From the perspective of anything orbiting any meaningful distance away, the difference between "mass near the black hole" and "mass consumed by the black hole" is irrelevant.  

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### Answer by username_9 on 2017-12-21. Score: 13

I once heard of a Japanese cartoon/movie/show where space pirates threatened to compress the planet Jupiter into a black hole and thus destroy half the Milky Way galaxy.

It sounds like an interesting idea, but... even if you could compress Jupiter into a black hole, its mass would remain the same, meaning that Jupiter (now a black hole) would still continue to move around our sun in its same orbit, and Jupiter's moons would still continue to orbit Jupiter as they did before.

Many people think that once a star collapses into a black hole, its "sucking power" (its gravitational force) increases. This is simply not the case. Believe it or not, many stars are *less* massive *after* they turn into a black hole than *before*, when they were shining stars. This is because, at the end of their lives, some stars shed a significant portion of their outer layer into space right before they collapse into a black hole.

I've read that if you compressed the Earth to the size of a cherry, its density would be so great that it would turn into a black hole. Assuming that were true and it was actually done, the black hole of Earth would still continue orbiting the sun once every year, and Earth's moon would continue to orbit the Earth about once every 29.5 days. (Now, the spin of the new black-hole-Earth about its axis would probably be different, but the time it would take to orbit the sun would not change.)

Surprisingly, once the Earth got compressed into a cherry-sized black hole, less space debris would fall into it than before (when the Earth was the size of... well, Earth). This is because the newly-formed black-hole-Earth would take up much less space (volume) and asteroids and comets would be more likely to miss the cherry-sized (or slightly-larger-than-cherry-sized) volume that, if not missed, would cause the debris to be sucked into the black hole.

If the debris missed the black-hole-Earth by even a kilometer (which might seem like a large distance to us, but is very miniscule in astronomical terms), it would be flung off in a different direction, possibly never to return.

So, basically, a common misconception people have regarding black holes is that nothing has more gravity than a black hole, and that stars that form into black holes all of a sudden have increased gravity and therefore get more "sucking power." This is simply not true. Black holes still have the same mass as before (sometimes less, depending on how they're formed), and how much "sucking power" they have is still dependent on how much mass they're made up of.

While it may be true that the most massive stars in the universe are indeed black holes (if you'd even call them *stars* at that point), there exist many stars that are more massive (and therefore have more "sucking power") than many black holes.

So the fact that our galaxy's center probably contains a super-massive black hole doesn't mean that the black hole would suck up any more matter than if it were the same amount of mass which happened to not be in black-hole-form.

> **Comments:**
> **username_10**: Another inaccuracy about space pirates destroying half the Milky Way with a black hole is the fact that any changes in Jupiter's gravitational field would not propagate faster than light and thus would take tens of thousands of years for all this destruction to be finished.  
> **username_11**: Also, isn’t destroying the galaxy sort of counter to the usual aims of piracy?  
> **username_12**: Nice and clear reminder of a common misconception. Thanks for pointing out that a black hole is no less no more than a gravitational object.  

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### Answer by username_13 on 2017-12-25. Score: 8

Gravity follows the law of inverse square. To put it simply if you double the distance from a gravity source you quarter is effect. So if you double the distance you are from the earth you feel 1/4g. It's important to note that as the distance increases it will never be 0, it will always be some non-zero value no matter the distance.

So at galactic distances the force of gravity the central black hole has very little effect.

This only explains part of it. The other part is conservation of angular momentum.

The force of gravity and the angular momentum is what is responsible for orbits. In orbital mechanics you raise your orbit by adding speed, not altitude. Your adding angular momentum which raises your orbit. To lower your orbit you reduce you speed which reduces your angular momentum and your altitude.

So for things to "fall" into a black hole they must be travailing at a speed where their orbit intersects the event horizon. This is rarely the case or those "things" wouldn't truly be in orbit to begin with. So the very fact that all the "stuff" that makes up the galaxy orbits the central black hole means that it cant just fall into it.

These 3 things are always in balance in a stable orbit, force of gravity, speed and altitude ( or distance from the gravity source ). If you change one of them the other 2 must also changes. If you decrease speed your altitude goes down, and the gravity increases. If you increase the gravity the speed must also increase or the altitude will decrease.

So you see things can't just fall into the black hole. That said it is my view that eventually everything in the galaxy will fall into the central black hole, however this will take many billions of years.

Of course this is overly simplifying things, and I am by no means an expert on this stuff. But it's something I can picture in my mind, the balance between momentum and gravity.

v


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### Answer by username_14 on 2017-12-20. Score: 6

You must also factor in the dark matter which is interacting gravitationally with all of the "hot matter" that can be seen in the galactic disk. Dark matter was discovered by carefully mapping the orbits of objects in galaxies and finding that the matter that could be seen could not account for the observed orbital motion. One of the mysteries of dark matter is that it is not pulled into the black hole the way hot matter is. The dark matter has the practical effect of balancing out some of the gravitational pull of the supermassive black hole at the galaxy's center.

> **Comments:**
> **username_15**: It depends on how the matter is distributed. Dark matter is generally thought to occur in a sphere around the galaxy. For a spherical distribution of matter, you only need to concern yourself with the portion interior to your orbit; what's outside won't affect you. So dark matter will still have the same result of pulling you inwards.  

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### Answer by username_16 on 2017-12-25. Score: 6

Well, I'm not a physics student, but I think people usually nurture the misconception of "sucking power" of a black hole for a reason.

Let us consider Newton's equation for gravity:

$F = {Gm\_im\_j\over r\_{ij}^2}$
for two bodies i and j, and $r\_{ij}$ is the distance between the centre of mass of two bodies.

Now, if the Sun today suddenly decided to become a black hole without shedding weight, it won't affect Earth's orbit, because even if Sun's volume has changed, $r\_{ij}$ remains constant.

The reason why Black Holes "suck" is because, since they occupy extremely less volume compared to planets and stars, you can get the $r\_{ij}$ component to be really really small.

Correct me if I'm wrong.


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### Answer by username_17 on 2017-12-21. Score: 5

For galaxies with large black holes, the surrounding matter is in *orbit* around the black hole(s), the same way that the moon orbits the earth.

The question is a direct analogy to "*Why doesn't the Moon fall to the ground?*" or "*Why don't the planets fall into the sun?*". The black hole is more massive than the Sun, but its effects are of the same type.

> **Comments:**
> **username_18**: That is not a typical situation at all. In the vast majority of cases the black hole is a tiny fraction of the total mass of the galaxy. There are some outliers, sure, but they are the exceptions.  
> **username_17**: Perhaps it's fairer to say that the black holes and other matter are all in orbits with each other.  Anyway, the important point is that there's a good analogy with the question most of us asked as children.  
> **username_18**: I'm sorry, but it's not a good analogy. What you're describing is literally a handful of cases out of countless millions.  

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### Answer by username_19 on 2017-12-21. Score: 5

One quick answer for your question would be event horizon or Schwarzschild radius. Anything which is fairly close to this radius/horizon will eventually be sucked up by the black hole.


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### Answer by username_20 on 2017-12-22. Score: 5

The simple answer is that everything else in the galaxy is going sideways fast enough to escape being sucked in. Instead, the force of the suck (if you like) causes the stars' paths to be pulled into a circle around the black hole.

This phenomenon is "orbit". As other answers pointed out, it's the same reason the Earth does not fall into the Sun, or the Moon fall onto the Earth, and why the International Space Station is hurtling along at around 17,150 miles per hour. They're all going sideways, the force of some large object is turning that sideways motion into circular motion, and if they weren't going fast enough then they'd curve ("fall") towards that large object and crash into it.

It's like if you whirl a bucket on the end of a string. The bucket is going sideways, but the string is pulling it towards you. The bucket doesn't fly off away from you because of the force from the string, and so it curves in a circle. The force from the string happens to not be enough to collapse the bucket inwards and hit you.


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### Answer by username_21 on 2017-12-25. Score: 5

Be patient, eventually it will unless the galaxy's rate of expansion exceeds the black hole's gravitational growth as it consumes the matter around it.

In that scenario the galaxy will eventually diffuse, with its matter continuing to travel away from the black hole until it encounters another galaxy, at which point it stands a good chance of eventually getting sucked into that's galaxy's black hole. Nothing survives forever.. :-)

> **Comments:**
> **username_22**: What makes you think that the galaxy is expanding? Sure, the universe is expanding, but that's only happening on the very large scale. Individual galaxies and even galaxy clusters aren't expanding because their gravity is stronger than the expansion at that scale.  

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### Answer by username_23 on 2017-12-22. Score: 5

This is a common misconception about black holes: that they somehow 'suck up' everything around them or pull things into them. In reality you could replace the Sun now with a black hole of the same mass and not notice any immediate difference. It's not like it would suddenly start hoovering in the planets around it, that's just not how it works.


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### Answer by username_24 on 2017-12-21. Score: -3

its all about ENTROPY which is proportional to the surface area of the event horizon of a black hole(see below for a heuristic quantum argument due to username_24/Wang as to why this is so).

Assuming a Schwarzschild solution gives a radius of 2Gm for the event horizon with m the black hole mass and G Newton's constant. Adding mass to a black hole thus increases its entropy. Given an isolated system of finite total energy, it has a finite maximum entropy which acts as an attractor for the dynamics of the system,placing a limit on the horizon.

J von Neumann defines a quantum version of entropy as follows: Let f be a normal state of a local algebra of observables O(D) acting on the Hilbert space H. Then we can write this f as a convex sum of pure states. For a system of finite energy this sum is finite since H is then finite dimensional
Von Neumann’s non-commutative equivalent of a partition is the density operator ie the weighted sum of the projections onto the minimal vector spaces corresponding to these pure states
Then we have the well-known equivalence;  
For such a normal state f, the von Neumann entropy is defined as the entropy of the weights . We interpret it as an (inverse) measure of the amount of information that the quantum system in a given state will yield through measurement. The larger the entropy of the quantum system, the less information can be extracted.
**The von Neumann Entropy of a Black Hole**
The measurement process cannot be performed by an external observer to elements within the interior, beyond the event horizon. We thus partition the event horizon of the black hole with elements each of area k squared, where k is the Planck length and assume the Planck area corresponds classically to the minimal projection of the pure vector state . Let N be the total finite number of partitions. By the ‘no hair’ hypothesis there is no preferred location on the event horizon, so that each partition element must have the same weighting. The von Neumann entropy of this partition is thus proportional to S the surface area of the black hole.

> **Comments:**
> **username_22**: While black hole entropy and the Beckenstein bound is an important and fascinating topic, I fail to see how it's particularly relevant to the OP's question.  
> **username_25**: This is a copypasta of https://www.researchgate.net/profile/Charles_Wang28/publication/313904636_Additional_Online_Material_For_%27Quantum_Ergodic_Theory_and_Diffeomorphism_Invariant_Quantum_States%27/data/58af52feaca2725b5411233c/additional-online-material-for-quantum-ergodic-theory.pdf with no relevance to the OP's question.  
> **username_24**: I improved my answer to take account of the kind comments  

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