<p>There are several sources of movement for galaxies.</p>

<p><strong>Galaxies may rotate</strong>.  Galaxies are formed essentially from matter collapsing under gravity into "clumps".  This process isn't uniform due to gravity from other clumps of matter and so it is very rare that all the particles in a single clump "fall" directly into it's centre.  This creates rotation (Angular Momentum) and so the eventual galaxy will rotate.  Note that some galaxies show very little overall rotation, with the individual stars orbiting the centre of the galaxy in a multiple directions.</p>

<p><strong>Galaxies interact with each other</strong>. Most galaxies reside within a <a href="https://en.wikipedia.org/wiki/Galaxy_cluster" rel="nofollow noreferrer">group or cluster</a> of galaxies, our galaxy is within a group called the <a href="https://en.wikipedia.org/wiki/Local_Group" rel="nofollow noreferrer">Local Group</a> with Andromeda and several ($\geq$52) dwarf galaxies.  These dwarf galaxies are usually part of a "satellite-subsystem" where they orbit a large galaxy under gravity.  These orbits are affected by the other local galaxies and occasionally some systems can be "expelled" due to the gravitational forces happening to speed the body up past the velocity required to escape the system.</p>

<p>The major galaxies in a group or cluster interact with each other, orbiting a centre of gravity.  This is due to the same mechanism as galaxy rotation.  This is usually a very dense area of galaxies, or a massive <a href="https://en.wikipedia.org/wiki/Brightest_cluster_galaxy" rel="nofollow noreferrer">Brightest Cluster Galaxy (BCG)</a>.  In the local group, the two main galaxies (our Milky Way and the Andromeda Galaxy) are getting closer together and will <a href="https://en.wikipedia.org/wiki/Andromeda%E2%80%93Milky_Way_collision" rel="nofollow noreferrer">collide</a> in approximately 4 billion years.</p>

<p><strong>The universe is expanding</strong>. The universe is expanding and so galaxies appear to be moving away from us in every direction.  We see this as <a href="https://en.wikipedia.org/wiki/Redshift" rel="nofollow noreferrer"><em>redshift</em></a>, a change in the wavelength of light as it reaches us due to the difference in speed between the origin an us.  This is not really anything to do with galaxies moving, and more to do with the fabric of the universe.  Whether this will continue, or whether the universe will stop expanding and collapse is a current <a href="https://en.wikipedia.org/wiki/Ultimate_fate_of_the_universe" rel="nofollow noreferrer">active area of research</a>.</p>

CC BY-SA 3.0
2017-04-07T20:19:18.187Z
Good answer, but regarding the last sentence, the data from the Planck and WMAP satellites have made it almost certain that the Universe will not collapse.
Sir Cumference
CC BY-SA 3.0
2017-04-10T07:34:27.990Z
Any source for that? WMAP and Planck measured the after-glow from the early universe, extrapolating that involves a huge number of models and estimations.  There is, for example, a whole research group at Nottingham (UK) still currently working on whether the Cosmological Constant is actually a correction to the models of gravity used or a separate entity.
Jonathan Twite
CC BY-SA 3.0
2017-04-10T14:45:46.490Z
Well, the Big Crunch can only happen in a closed (positively curved) universe where $\ddot{a} < 0$. According to [Bennett et al.](https://arxiv.org/abs/1212.5225), "...the universe is close to flat/Euclidean ($Ω_k = −0.0027^{+0.0039}_{−0.0038}$)." Finally, we have determined $\ddot{a} > 0$ in our own Universe. It shouldn't be possible for our Universe to collapse, since we don't live in any Friedmann model, let alone that particular Friedmann model.
Sir Cumference
CC BY-SA 3.0
2017-04-05T08:53:53.810Z
2017-04-05T08:53:53.810Z
Jonathan Twite
<p>I don't understand and I haven't understood for a while.
How is it that all the galaxies in the universe are moving, how they are moving and how fast?</p>

CC BY-SA 3.0
2017-04-05T05:24:30.113Z
Are you referring to 1) their "internal" movement, i.e. how stars move around in galaxies (which is caused by gravity), 2) their movement through space (which is also caused by gravity), or 3) their recession from each other (which is caused by the expansion of the Universe)?
pela
CC BY-SA 3.0
2017-04-05T05:30:14.270Z
How the galaxies move altogether.
natural
CC BY-SA 3.0
2017-04-05T05:54:21.297Z
@natural You didn't answer pela's question. 1) is very different from 2) and 3).
Sir Cumference
<galaxy><movement>
How are galaxies moving so much and why are they moving?
natural
# How are galaxies moving so much and why are they moving?

(Asked by: username_0 on 2017-04-05)

I don't understand and I haven't understood for a while.
How is it that all the galaxies in the universe are moving, how they are moving and how fast?

**Tags:** galaxy, movement

> **Comments:**
> **username_1**: Are you referring to 1) their "internal" movement, i.e. how stars move around in galaxies (which is caused by gravity), 2) their movement through space (which is also caused by gravity), or 3) their recession from each other (which is caused by the expansion of the Universe)?  
> **username_0**: How the galaxies move altogether.  
> **username_2**: @username_0 You didn't answer username_1's question. 1) is very different from 2) and 3).  

---

## 1 answers

### Answer by username_3 on 2017-04-05. Score: 2

There are several sources of movement for galaxies.

**Galaxies may rotate**. Galaxies are formed essentially from matter collapsing under gravity into "clumps". This process isn't uniform due to gravity from other clumps of matter and so it is very rare that all the particles in a single clump "fall" directly into it's centre. This creates rotation (Angular Momentum) and so the eventual galaxy will rotate. Note that some galaxies show very little overall rotation, with the individual stars orbiting the centre of the galaxy in a multiple directions.

**Galaxies interact with each other**. Most galaxies reside within a [group or cluster](https://en.wikipedia.org/wiki/Galaxy_cluster) of galaxies, our galaxy is within a group called the [Local Group](https://en.wikipedia.org/wiki/Local_Group) with Andromeda and several ($\geq$52) dwarf galaxies. These dwarf galaxies are usually part of a "satellite-subsystem" where they orbit a large galaxy under gravity. These orbits are affected by the other local galaxies and occasionally some systems can be "expelled" due to the gravitational forces happening to speed the body up past the velocity required to escape the system.

The major galaxies in a group or cluster interact with each other, orbiting a centre of gravity. This is due to the same mechanism as galaxy rotation. This is usually a very dense area of galaxies, or a massive [Brightest Cluster Galaxy (BCG)](https://en.wikipedia.org/wiki/Brightest_cluster_galaxy). In the local group, the two main galaxies (our Milky Way and the Andromeda Galaxy) are getting closer together and will [collide](https://en.wikipedia.org/wiki/Andromeda%E2%80%93Milky_Way_collision) in approximately 4 billion years.

**The universe is expanding**. The universe is expanding and so galaxies appear to be moving away from us in every direction. We see this as [*redshift*](https://en.wikipedia.org/wiki/Redshift), a change in the wavelength of light as it reaches us due to the difference in speed between the origin an us. This is not really anything to do with galaxies moving, and more to do with the fabric of the universe. Whether this will continue, or whether the universe will stop expanding and collapse is a current [active area of research](https://en.wikipedia.org/wiki/Ultimate_fate_of_the_universe).

> **Comments:**
> **username_2**: Good answer, but regarding the last sentence, the data from the Planck and WMAP satellites have made it almost certain that the Universe will not collapse.  
> **username_3**: Any source for that? WMAP and Planck measured the after-glow from the early universe, extrapolating that involves a huge number of models and estimations.  There is, for example, a whole research group at Nottingham (UK) still currently working on whether the Cosmological Constant is actually a correction to the models of gravity used or a separate entity.  
> **username_2**: Well, the Big Crunch can only happen in a closed (positively curved) universe where $\ddot{a} < 0$. According to [Bennett et al.](https://arxiv.org/abs/1212.5225), "...the universe is close to flat/Euclidean ($Ω_k = −0.0027^{+0.0039}_{−0.0038}$)." Finally, we have determined $\ddot{a} > 0$ in our own Universe. It shouldn't be possible for our Universe to collapse, since we don't live in any Friedmann model, let alone that particular Friedmann model.  

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