<p>I assume you're asking about central supermassive black holes (SMBHs, one per galaxy), not stellar-mass black holes.</p>

<p>The answer is yes, but what actually happens is the two SMBHs have to merge first, and then the resulting <em>combined</em> SMBH can sometimes be ejected from the combined (merged) galaxy.</p>

<p>[Edited to add: Since you've updated the question with a series of diagrams, I should state explicitly that the scenario suggested by the diagrams -- stars in smaller galaxy merge into big galaxy, but SMBH continues on almost unaffected -- is not physically possible. Most of the stars from the smaller galaxy will not end up in the center of the big galaxy, but because of <a href="https://en.wikipedia.org/wiki/Dynamical_friction" rel="nofollow noreferrer">dynamical friction</a>, the SMBH <em>will</em>.]</p>

<p><a href="https://www.nasa.gov/feature/goddard/2017/gravitational-wave-kicks-monster-black-hole-out-of-galactic-core" rel="nofollow noreferrer">This NASA press release</a> from 2017 describes the discovery of a quasar apparently ejected from a recently merged galaxy. I'll go ahead and quote their description of the suggested mechanism (this possibility has been suggested by theoretical studies going back at least ten or fifteen years):</p>

<blockquote>
  <p>According to their theory, two galaxies merge, and their black holes
  settle into the center of the newly formed elliptical galaxy. As the
  black holes whirl around each other, gravity waves are flung out like
  water from a lawn sprinkler. The hefty objects move closer to each
  other over time as they radiate away gravitational energy. If the two
  black holes do not have the same mass and rotation rate, they emit
  gravitational waves more strongly along one direction. When the two
  black holes collide, they stop producing gravitational waves. The
  newly merged black hole then recoils in the opposite direction of the
  strongest gravitational waves and shoots off like a rocket.</p>
</blockquote>

<p>Since most massive galaxies -- including those that have undergone major mergers in the past -- have a SMBH in their center, the gravitational recoil usually isn't strong enough to eject the SMBH; instead, the SMBH loses energy to the stars in the inner part of the merged galaxy via dynamical friction, and settles back into the center. But it appears that sometimes there's enough of a kick to allow the SMBH to escape.</p>

<p>Another possibility is that if two galaxies merge and their SMBHs form a binary, and then <em>another</em> galaxy (with its own SMBH) merges <em>before</em> the previous two SMBHs have actually merged, then you can have a three-body interaction between the late-arrival SMBH and the binary SMBH, which could result in one of the SMBHs being ejected. But this requires the right timing, and probably doesn't happen very often.</p>

CC BY-SA 4.0
2018-06-29T11:30:22.690Z
That's a great answer Peter. I do think there's something of an issue as regards how black holes move in a gravitational field, but that's one for another day.
John Duffield
CC BY-SA 4.0
2018-06-27T21:36:57.390Z
2018-06-30T11:49:57.587Z
2018-06-30T11:49:57.587Z
Peter Erwin
<p>Yes, and in fact a mechanism somewhat like this has probably dumped a large number of BHs into intergalactic space.</p>

<p>Black holes tend to settle towards the center of galaxies (an effect of dynamical friction). As they settle, they "cool" by evaporation. The chaos of BHs orbiting the center of mass all interact, especially when two of them approach closely. Depending on the geometry of the near-miss, one BH can gain energy at the expense of the other. One swings into a larger orbit and the other goes into a smaller orbit.</p>

<p>Sometime the larger orbit is hyperbolic and the BH is thrown right out of the galaxy.  This removes orbital energy from the assemblage of BHs and the whole thing shrinks a bit and encounters become a bit more common.  In the end, many of the original set of BHs are thrown out into intergalactic space.</p>

<p>How many?  No one knows yet. We have good evidence of a single very large BH (>10<sup>6</sup> solar masses) at the center of the Milky Way, but recent results have suggested there may be as many as 10,000 smaller BHs (~10 solar masses each) in orbit around it.</p>

<p>If the latter is right, there may be a <em>lot</em> of BHs wandering intergalactic space!</p>

CC BY-SA 4.0
2018-06-27T21:16:14.540Z
I think the question is about *central supermassive black holes*, not ordinary stellar-mass black holes.
Peter Erwin
CC BY-SA 4.0
2018-06-27T21:24:22.213Z
In any case, your analysis ignores interactions with stars, which will outnumber the black holes; since most stars are low mass, the tendency will be for the black holes to lose energy and sink towards the center, with the lower mass stars gaining energy. And two-body interactions only take place in *very* dense environments. This is not an effective way of ejecting black holes.
Peter Erwin
CC BY-SA 4.0
2018-06-27T21:29:54.530Z
That doesn't change anything qualitatively: BHs still get flung out of the galaxy, because the denser they are towards the center, the more frequent the close interactions that do the flinging and this compensates for the somewhat higher escape velocity from closer in.
Mark Olson
CC BY-SA 4.0
2018-06-27T21:49:47.347Z
No, this will not eject BHs. Because the interactions involve stars with a range of masses (mostly $<$ the BHs), there will be mass segregation: more massive objects will lose energy and sink to smaller radii, while less massive objects will gain energy. The result will be a concentration of the BHs and massive stars towards the center of the galaxy nucleus.
https://en.wikipedia.org/wiki/Mass_segregation_(astronomy)
Peter Erwin
CC BY-SA 4.0
2018-06-27T19:44:55.457Z
2018-06-27T19:44:55.457Z
Mark Olson
<p>Could two galaxies (one big and one small)intersect at a velocity to allow the smaller black hole to escape but not the galaxy around it?</p>

<p><a href="https://i.sstatic.net/mheGW.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/mheGW.jpg" alt="enter image description here"></a></p>

CC BY-SA 4.0
2018-06-29T12:58:00.857Z
In regards to the drawing that your questions has been updated your question with: no, that wouldn't happen (that would require that the smaller galaxy's central SMBH responded to gravity in a completely different way from the stars).
Peter Erwin
<black-hole><galaxy><mass><velocity><density>
Can "rogue" supermassive black holes be made this way?
Muze
# Can "rogue" supermassive black holes be made this way?

(Asked by: username_0 on 2018-06-27)

Could two galaxies (one big and one small)intersect at a velocity to allow the smaller black hole to escape but not the galaxy around it?

[![enter image description here](https://i.sstatic.net/mheGW.jpg)](https://i.sstatic.net/mheGW.jpg)

**Tags:** black-hole, galaxy, mass, velocity, density
> **Comments:**
> **username_1**: In regards to the drawing that your questions has been updated your question with: no, that wouldn't happen (that would require that the smaller galaxy's central SMBH responded to gravity in a completely different way from the stars).  

---

## 2 answers

### Answer by username_1 on 2018-06-27. Score: 10

I assume you're asking about central supermassive black holes (SMBHs, one per galaxy), not stellar-mass black holes.

The answer is yes, but what actually happens is the two SMBHs have to merge first, and then the resulting *combined* SMBH can sometimes be ejected from the combined (merged) galaxy.

[Edited to add: Since you've updated the question with a series of diagrams, I should state explicitly that the scenario suggested by the diagrams -- stars in smaller galaxy merge into big galaxy, but SMBH continues on almost unaffected -- is not physically possible. Most of the stars from the smaller galaxy will not end up in the center of the big galaxy, but because of [dynamical friction](https://en.wikipedia.org/wiki/Dynamical_friction), the SMBH *will*.]

[This NASA press release](https://www.nasa.gov/feature/goddard/2017/gravitational-wave-kicks-monster-black-hole-out-of-galactic-core) from 2017 describes the discovery of a quasar apparently ejected from a recently merged galaxy. I'll go ahead and quote their description of the suggested mechanism (this possibility has been suggested by theoretical studies going back at least ten or fifteen years):

> According to their theory, two galaxies merge, and their black holes
> settle into the center of the newly formed elliptical galaxy. As the
> black holes whirl around each other, gravity waves are flung out like
> water from a lawn sprinkler. The hefty objects move closer to each
> other over time as they radiate away gravitational energy. If the two
> black holes do not have the same mass and rotation rate, they emit
> gravitational waves more strongly along one direction. When the two
> black holes collide, they stop producing gravitational waves. The
> newly merged black hole then recoils in the opposite direction of the
> strongest gravitational waves and shoots off like a rocket.

Since most massive galaxies -- including those that have undergone major mergers in the past -- have a SMBH in their center, the gravitational recoil usually isn't strong enough to eject the SMBH; instead, the SMBH loses energy to the stars in the inner part of the merged galaxy via dynamical friction, and settles back into the center. But it appears that sometimes there's enough of a kick to allow the SMBH to escape.

Another possibility is that if two galaxies merge and their SMBHs form a binary, and then *another* galaxy (with its own SMBH) merges *before* the previous two SMBHs have actually merged, then you can have a three-body interaction between the late-arrival SMBH and the binary SMBH, which could result in one of the SMBHs being ejected. But this requires the right timing, and probably doesn't happen very often.

> **Comments:**
> **username_2**: That's a great answer Peter. I do think there's something of an issue as regards how black holes move in a gravitational field, but that's one for another day.  

---

### Answer by username_3 on 2018-06-27. Score: 4

Yes, and in fact a mechanism somewhat like this has probably dumped a large number of BHs into intergalactic space.

Black holes tend to settle towards the center of galaxies (an effect of dynamical friction). As they settle, they "cool" by evaporation. The chaos of BHs orbiting the center of mass all interact, especially when two of them approach closely. Depending on the geometry of the near-miss, one BH can gain energy at the expense of the other. One swings into a larger orbit and the other goes into a smaller orbit.

Sometime the larger orbit is hyperbolic and the BH is thrown right out of the galaxy. This removes orbital energy from the assemblage of BHs and the whole thing shrinks a bit and encounters become a bit more common. In the end, many of the original set of BHs are thrown out into intergalactic space.

How many? No one knows yet. We have good evidence of a single very large BH (>106 solar masses) at the center of the Milky Way, but recent results have suggested there may be as many as 10,000 smaller BHs (~10 solar masses each) in orbit around it.

If the latter is right, there may be a *lot* of BHs wandering intergalactic space!

> **Comments:**
> **username_1**: I think the question is about *central supermassive black holes*, not ordinary stellar-mass black holes.  
> **username_1**: In any case, your analysis ignores interactions with stars, which will outnumber the black holes; since most stars are low mass, the tendency will be for the black holes to lose energy and sink towards the center, with the lower mass stars gaining energy. And two-body interactions only take place in *very* dense environments. This is not an effective way of ejecting black holes.  
> **username_3**: That doesn't change anything qualitatively: BHs still get flung out of the galaxy, because the denser they are towards the center, the more frequent the close interactions that do the flinging and this compensates for the somewhat higher escape velocity from closer in.  
> **username_1**: No, this will not eject BHs. Because the interactions involve stars with a range of masses (mostly $<$ the BHs), there will be mass segregation: more massive objects will lose energy and sink to smaller radii, while less massive objects will gain energy. The result will be a concentration of the BHs and massive stars towards the center of the galaxy nucleus. https://en.wikipedia.org/wiki/Mass_segregation_(astronomy)  

---

