Question about expanding universe VS gravity pull.

Click For Summary

Discussion Overview

The discussion revolves around the relationship between the expansion of the universe and the gravitational pull of celestial bodies. Participants explore concepts related to the Big Bang, escape velocity, and the implications of gravitational forces on cosmic expansion, touching on theoretical scenarios and observational studies.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Christian introduces the idea that as the universe expands, gravity from stars and planets should slow this expansion, questioning if science can calculate when gravity will overcome the expansion.
  • Another participant clarifies that if the universe is expanding at greater than escape velocity, it will always do so, and that gravity weakens as galaxies move further apart, suggesting the expansion will not stop.
  • There is a mention of a study from the 1990s indicating that the universe's expansion is actually accelerating due to an unknown force termed "dark energy," which challenges the idea of a slowing expansion.
  • Christian raises a concern about the eventual separation of galaxies, questioning if gravitational pull will become negligible enough to lead to isolated "mini universes." This point is reiterated with the assertion that gravitational pull never ceases but may become too weak to counteract expansion.
  • A later reply discusses the implications of accelerating expansion, suggesting that after a significant time, regions of the universe will become isolated from one another, leading to a scenario where contact between these regions is impossible.

Areas of Agreement / Disagreement

Participants express differing views on the effects of gravity on the universe's expansion, with some arguing that gravity will eventually stop the expansion while others assert that the expansion is accelerating and will continue indefinitely. The discussion remains unresolved regarding the long-term fate of the universe and the nature of gravitational influence at vast distances.

Contextual Notes

Participants reference observational studies and theoretical models without reaching consensus on the implications of gravitational forces versus cosmic expansion. The discussion highlights uncertainties regarding the nature of dark energy and the long-term behavior of the universe.

Cloengaa
Messages
3
Reaction score
0
Hello all. I am a newcomer on the forum and no major math or astronomy knower.

But I have often thought about this issue I would like to ask about here.

From what I understand the Big Bang happened from a singularity expanding outwards (or exploding). As the speed of light is considered a constant, when the singularity expanded it can only reach the speed of light.

Now as the universe expands bodies are made, stars, planets and all these bodies have a gravity pull on the expanding universe.

So as now the expansion speed is bigger than the gravity pull of these bodies, but the gravity pull must slow the expansion down.

So should science not be able to calculate when the expanse will stop and the gravity pull will be bigger than the escape velocity ?

I know this might sound stupid or like I am a real dummie, but I am trying to learn more so please have patience with me.

Regards

Christian
 
Astronomy news on Phys.org
If the universe were expanding at greater than escape velocity now, it would always be doing so. This is what escape velocity is. As the universe expands the individual galaxies move further apart, meaning that their gravitational hold on each other weakens. The expansion would slow but never slow to a stop.

If however, the it is expanding at less than escape velocity, eventually gravity will overcome the expansion and it will stop and then reverse to a "big crunch".

In the 1990's a study was done to determine just which one of these scenarios was right. By comparing a galaxies distance from us to its speed, they could plot out the rate of expansion over time ( Remember, the further a galaxy is away from us, the longer it takes for the light from it to reach us. We are seeing the galaxy as it was when the light left, not as it is now. This allows us to peer into the past of the Universe.) In this way we could determine the rate at which the universe's expansion changes over time, which allows us to figure out whether or not the expansion is slowing fast enough to eventually stop or not.

The odd thing was that they found that the expansion wasn't slowing at all, it was in fact, speeding up. It was as if something were acting against gravity over long distances, pushing the universe apart. This something was given the term "dark energy", and its exact nature in under current examination.

The upshot is that, by our best current knowledge, the universe will continue to expand forever, and it will never come to a stop.
 
Thanks Janus for the response.

I have heard about the expanding faster issue. What I am thinking about that is at some point the gravitational pulls from foreign galaxis and bodies will be so far from each other there will be no pull what so ever. Does this not mean that the universe will not continue to "hang together" as ONE unit, but split up in mini universes with nothing in between them ?
 
What I am thinking about that is at some point the gravitational pulls from foreign galaxis and bodies will be so far from each other there will be no pull what so ever.
Gravitational pull never ceases. But it might be too weak to stop the expansion.
Does this not mean that the universe will not continue to "hang together" as ONE unit, but split up in mini universes with nothing in between them ?
Distances get larger amd larger, that doesn't necessarily mean that portions of the universe get separated without any chance of contacting each other.
It's different with accelerating expansion, however. After ~100 bn years (according to the standard model), the universe will be split up into infinitely many regions without contact to their neighbours. One of those regions will be our vicinity, the supercluster we're in.
We'll see/measure an event horizon surrounding this region, beyond which we can't see.
 

Similar threads

  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 4 ·
Replies
4
Views
7K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 24 ·
Replies
24
Views
3K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 6 ·
Replies
6
Views
2K