<p>Right now the expansion of space is only observed on scales like that of galaxies and the entire universe. We say that with the fancy term <em>globally</em>. Expansion of space does not take place within galaxies at least for now.</p>
<p>As pela has rightfully noted in the comments, for now the gravitation of galaxies, stars etc. is strong enough to overcome the expansion of the universe. But as General Relativity tells us gravity is <em>local</em>, that is, it only affects objects that are considerably close. So, on large scales expansion continues. (I am no expert, but I think that the reason for expansion not happening within galaxies out smaller systems is that the matter and energy is more dense, resolution by in stronger gravitational fields).</p>
<p>It is hypothesized that the universe may end with a big rip: this means that the expansion eventually would start to affect galaxies. Galaxies, star systems, planets and eventually atoms will be ripped apart due to the expansion of space. When and if that happens, not only gravity but not even electromagnetism or the strong force would work to overcome the mighty expansion.</p>
<p>But this situation is highly hypothetical and maybe it won't even happen. So for now, the answer is no: the expansion of the universe could not affect gravitational acceleration.</p>

CC BY-SA 4.0
2020-06-18T14:03:43.187Z
2020-06-18T14:03:43.187Z
PNS
<p>My two cents:</p>
<p>By how much amount the space &quot;stretches&quot; between the two hypothetical bodies you pose, is measured by redshift of a hypothetical photon traveling between these two bodies.  At this point, the dark energy doesn't dominate scales where what we call &quot;acceleration due to gravity&quot; makes sense, and the only redshift that the photon undergoes is through the classical STR/GTR effects.</p>
<p>To see the effects of dark energy (right now, at least), one would need to be on scales where individual objects are indistinguishable and what is seen is just a homogenous &quot;cosmological fluid&quot;.  At that point, since there is no way of telling one object from another, there exists no concept of an acceleration due to gravity.  So, at small scales, the answer is no.</p>
<p>However, one could pose the question in a different manner: in the cosmological fluid, does gravity play a role?  And if it does, is there a regime where the gravity (from local structures collapsing) is similar to the &quot;force&quot; of expansion from the universe expanding?  In that case, the answer is yes to both.  <a href="https://astronomy.stackexchange.com/questions/50038/calculating-the-turnaround-point-where-expansion-dominates-over-gravity">See this discussion for example</a></p>

CC BY-SA 4.0
2022-07-28T21:49:12.600Z
2022-07-28T21:49:12.600Z
terribleGuitarPlayer
<p>When we thought the Cosmological Constant was zero, the solution for the motion of an object near a galaxy was Newtonian.  That is, where densities are low, space-time becomes curved by gravity in such a way that the Newtonian orbits are correct (although space may no longer be exactly Euclidean, ie. flat).  One only needed to worry about GR effects near a BH or other compact object.  Now, with non-zero cosmological constant, that term must be taken into account.  It acts as a pressure (or negative density) that reduces the inward acceleration between two masses.  However, it’s effects are relatively important only on very large scales where the local mass density drops to below critical density.  As it turns out, the cosmological constant is at just the right level to keep the universe almost completely flat, ie. space is not curved on the largest scales (or very very close to flat).</p>
<p>How does the expansion of space come into this?  Well, after you solve the Friedmann Equations for the cosmological orbits, you can look at the expanded distances between galaxies and say that space must have been created anew.  Space is not a force and has no force.</p>

CC BY-SA 4.0
2022-07-28T21:08:28.917Z
Does not look right at all to me, especially "with non-zero cosmological constant, that term [from GR] must be taken into account." GR effects are observable **regardless** of the cosmological constant: Mercury's orbit precession, GPS satellite corrections, etc all need GTR; they don't need a non-zero cosmological constant!
terribleGuitarPlayer
CC BY-SA 4.0
2022-07-30T16:18:12.113Z
I’m saying the universe follows GR everywhere, but there are no terms of GR dealing with what space is doing.  Rather, we interpret the GR solution of an expanding universe as space expanding.  The Sun and the Earth are compact objects compared to large scale structure where GR with $\Lambda=0$ becomes Newtonian.
eshaya
CC BY-SA 4.0
2022-07-26T21:16:13.543Z
2022-08-01T15:04:49.070Z
2022-08-01T15:04:49.070Z
eshaya
<p>I was wondering if theoretically the universe expanding affects speed or acceleration due to gravity, compared to if space weren't accelerating. </p>

<p>The way I have it in my head, something is falling towards a planet with gravity G acting upon it. It's been falling for T amount of time and has gone X distance with Y left to go. Currently the universe is expanding, so the distance between its starting and ending point is a very tiny bit longer when it arrives than when it started, either affecting its distance traveled at time T, or its speed at time T.  Compare this to a non-expanding universe where the distance between start and end remains the same, no matter what point in time you choose. </p>

<p>I know that local gravity forces and atomic forces greatly overpower expansion forces so galaxies, solar systems, planets, and watermelons don't just fly apart. I'm just wondering if the value of either gravitational acceleration, or an object's speed could theoretically be changed slightly due to cosmic expansion. </p>

CC BY-SA 3.0
2016-06-09T14:42:20.493Z
Good question, but local gravity forces not only overpower the expansion of the Universe on small scales, it actually prevents it. That is, inside galaxies the Universe doesn't expand _at all_. So the answer is no.
pela
CC BY-SA 3.0
2016-06-09T16:54:51.523Z
@pela That's a bit misleading. They do counter it with gravity, but because the amount of dark energy in the Universe is increasing, they will eventually expand. Not to mention, as far as I know, space is still being created between stars in galaxies — but they are still held together by gravity.
Sir Cumference
CC BY-SA 3.0
2016-06-10T16:48:23.083Z
@SirCumference: On second thought, I don't know to be honest, or at least I think it's impossible to differentiate observationally. Space expands because the initial kick (Big Bang) was larger than the mutual attraction of stuff (and lately because of dark energy). By Birkhoff's theorem, an overdensity (at least a spherical one) can be treated as a mini-universe, independent of the rest of the Universe. So in places with enough matter, space is "held together" by gravity, preventing expansion. That's the standard discription at least, but I'm not sure it's true…
pela
CC BY-SA 3.0
2016-06-10T17:07:37.723Z
@pela If I recall, space itself is expanding; the objects aren't moving away from each other in the traditional sense, but are becoming more distant, since space is actually being created in between the matter. In fact, they can actually drift away from each other faster than light; Einstein said nothing can move *though* space FTL, but here, space is literally being created between them. Pretty much, gravity could hold the objects close together, but space between them will expand independently.

Though, I'm not 100% sure if this info is correct, but this is from what I've heard.
Sir Cumference
CC BY-SA 3.0
2016-06-10T19:28:15.777Z
@SirCumference Completely true; space expands, and galaxies follows along, and for sufficiently large distance, galaxies recede faster than light. But until space was small enough that dark energy played no significant role, the expansion was decelerated because of the mass in space. So matter prevents expansion. Whether or not it prevents it completely inside sufficiently dense regions is debatable, or not known. This is at least the conclusion I and a few colleagues reached today (but none of us are general relativists, only galaxy/dark matter astrophysicists, so I better stop talking :) )
pela
CC BY-SA 3.0
2016-06-10T19:53:04.573Z
@pela Better than me, I'm in high school and I just read it for fun :)
Sir Cumference
CC BY-SA 3.0
2016-06-10T21:35:37.257Z
That's a good start :)
pela
CC BY-SA 3.0
2016-06-14T01:14:36.497Z
I would think that space must not expand "locally" (where there is sufficient density of matter) or else a "meter stick" would expand at the same rate and we wouldn't notice. Sorry, not a cosmologist..
Jack R. Woods
CC BY-SA 3.0
2016-06-21T11:29:10.003Z
@JackR.Woods The more space there is between two objects, the more space there is to expand. That's why farther objects drift away from us more quickly, as far as I know.
Sir Cumference
<gravity><space-time><expansion>
Theoretically could the expansion of the universe affect acceleration due to gravity?
Artemis
# Theoretically could the expansion of the universe affect acceleration due to gravity?

(Asked by: username_0 on 2016-06-09)

I was wondering if theoretically the universe expanding affects speed or acceleration due to gravity, compared to if space weren't accelerating.

The way I have it in my head, something is falling towards a planet with gravity G acting upon it. It's been falling for T amount of time and has gone X distance with Y left to go. Currently the universe is expanding, so the distance between its starting and ending point is a very tiny bit longer when it arrives than when it started, either affecting its distance traveled at time T, or its speed at time T. Compare this to a non-expanding universe where the distance between start and end remains the same, no matter what point in time you choose.

I know that local gravity forces and atomic forces greatly overpower expansion forces so galaxies, solar systems, planets, and watermelons don't just fly apart. I'm just wondering if the value of either gravitational acceleration, or an object's speed could theoretically be changed slightly due to cosmic expansion.

**Tags:** gravity, space-time, expansion
> **Comments:**
> **username_1**: Good question, but local gravity forces not only overpower the expansion of the Universe on small scales, it actually prevents it. That is, inside galaxies the Universe doesn't expand _at all_. So the answer is no.  
> **username_2**: @pela That's a bit misleading. They do counter it with gravity, but because the amount of dark energy in the Universe is increasing, they will eventually expand. Not to mention, as far as I know, space is still being created between stars in galaxies — but they are still held together by gravity.  
> **username_1**: @SirCumference: On second thought, I don't know to be honest, or at least I think it's impossible to differentiate observationally. Space expands because the initial kick (Big Bang) was larger than the mutual attraction of stuff (and lately because of dark energy). By Birkhoff's theorem, an overdensity (at least a spherical one) can be treated as a mini-universe, independent of the rest of the Universe. So in places with enough matter, space is "held together" by gravity, preventing expansion. That's the standard discription at least, but I'm not sure it's true…  
> **username_2**: @pela If I recall, space itself is expanding; the objects aren't moving away from each other in the traditional sense, but are becoming more distant, since space is actually being created in between the matter. In fact, they can actually drift away from each other faster than light; Einstein said nothing can move *though* space FTL, but here, space is literally being created between them. Pretty much, gravity could hold the objects close together, but space between them will expand independently.  Though, I'm not 100% sure if this info is correct, but this is from what I've heard.  
> **username_1**: @SirCumference Completely true; space expands, and galaxies follows along, and for sufficiently large distance, galaxies recede faster than light. But until space was small enough that dark energy played no significant role, the expansion was decelerated because of the mass in space. So matter prevents expansion. Whether or not it prevents it completely inside sufficiently dense regions is debatable, or not known. This is at least the conclusion I and a few colleagues reached today (but none of us are general relativists, only galaxy/dark matter astrophysicists, so I better stop talking :) )  
> **username_2**: @pela Better than me, I'm in high school and I just read it for fun :)  
> **username_1**: That's a good start :)  
> **username_3**: I would think that space must not expand "locally" (where there is sufficient density of matter) or else a "meter stick" would expand at the same rate and we wouldn't notice. Sorry, not a cosmologist..  
> **username_2**: @JackR.Woods The more space there is between two objects, the more space there is to expand. That's why farther objects drift away from us more quickly, as far as I know.  

---

## 3 answers

### Answer by username_4 on 2020-06-18. Score: 1

Right now the expansion of space is only observed on scales like that of galaxies and the entire universe. We say that with the fancy term *globally*. Expansion of space does not take place within galaxies at least for now.

As pela has rightfully noted in the comments, for now the gravitation of galaxies, stars etc. is strong enough to overcome the expansion of the universe. But as General Relativity tells us gravity is *local*, that is, it only affects objects that are considerably close. So, on large scales expansion continues. (I am no expert, but I think that the reason for expansion not happening within galaxies out smaller systems is that the matter and energy is more dense, resolution by in stronger gravitational fields).

It is hypothesized that the universe may end with a big rip: this means that the expansion eventually would start to affect galaxies. Galaxies, star systems, planets and eventually atoms will be ripped apart due to the expansion of space. When and if that happens, not only gravity but not even electromagnetism or the strong force would work to overcome the mighty expansion.

But this situation is highly hypothetical and maybe it won't even happen. So for now, the answer is no: the expansion of the universe could not affect gravitational acceleration.


---

### Answer by username_5 on 2022-07-28. Score: 0

My two cents:

By how much amount the space "stretches" between the two hypothetical bodies you pose, is measured by redshift of a hypothetical photon traveling between these two bodies. At this point, the dark energy doesn't dominate scales where what we call "acceleration due to gravity" makes sense, and the only redshift that the photon undergoes is through the classical STR/GTR effects.

To see the effects of dark energy (right now, at least), one would need to be on scales where individual objects are indistinguishable and what is seen is just a homogenous "cosmological fluid". At that point, since there is no way of telling one object from another, there exists no concept of an acceleration due to gravity. So, at small scales, the answer is no.

However, one could pose the question in a different manner: in the cosmological fluid, does gravity play a role? And if it does, is there a regime where the gravity (from local structures collapsing) is similar to the "force" of expansion from the universe expanding? In that case, the answer is yes to both. [See this discussion for example](https://astronomy.stackexchange.com/questions/50038/calculating-the-turnaround-point-where-expansion-dominates-over-gravity)


---

### Answer by username_6 on 2022-07-26. Score: 0

When we thought the Cosmological Constant was zero, the solution for the motion of an object near a galaxy was Newtonian. That is, where densities are low, space-time becomes curved by gravity in such a way that the Newtonian orbits are correct (although space may no longer be exactly Euclidean, ie. flat). One only needed to worry about GR effects near a BH or other compact object. Now, with non-zero cosmological constant, that term must be taken into account. It acts as a pressure (or negative density) that reduces the inward acceleration between two masses. However, it’s effects are relatively important only on very large scales where the local mass density drops to below critical density. As it turns out, the cosmological constant is at just the right level to keep the universe almost completely flat, ie. space is not curved on the largest scales (or very very close to flat).

How does the expansion of space come into this? Well, after you solve the Friedmann Equations for the cosmological orbits, you can look at the expanded distances between galaxies and say that space must have been created anew. Space is not a force and has no force.

> **Comments:**
> **username_5**: Does not look right at all to me, especially "with non-zero cosmological constant, that term [from GR] must be taken into account." GR effects are observable **regardless** of the cosmological constant: Mercury's orbit precession, GPS satellite corrections, etc all need GTR; they don't need a non-zero cosmological constant!  
> **username_6**: I’m saying the universe follows GR everywhere, but there are no terms of GR dealing with what space is doing.  Rather, we interpret the GR solution of an expanding universe as space expanding.  The Sun and the Earth are compact objects compared to large scale structure where GR with $\Lambda=0$ becomes Newtonian.  

---

