Gravity Between Two Stars 45 Billion Light Years Away?

Click For Summary

Discussion Overview

The discussion revolves around the gravitational interaction between two stars located 45 billion light years apart, exploring the implications of distance on gravitational force in both theoretical and real-world contexts. Participants examine the mathematical framework of gravity, its practical limitations, and the conceptual challenges of applying models to extreme scenarios.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant suggests that in the equation F = GMm/r^2, as r approaches infinity, gravitational force remains a non-zero value mathematically, but questions its real-world applicability.
  • Another participant asserts that gravity has an infinite reach in both Newtonian and relativistic frameworks, indicating that its effects are always non-zero.
  • A different viewpoint emphasizes that while the equation holds under certain conditions, practical limitations exist due to the inability to create an empty space devoid of gravitational influences for testing.
  • One participant clarifies that the concept of "close to infinity" is misleading, as any finite distance remains infinitely far from infinity.
  • Another participant notes that while theoretical predictions may yield a small non-zero gravitational force, practical measurement limitations can render such values negligible.
  • A further contribution highlights the importance of considering the validity of models based on parameter values, referencing issues in quantum field theories and their relevance to Newtonian physics.

Areas of Agreement / Disagreement

Participants express differing views on the implications of distance on gravitational force, with some asserting non-zero effects at large distances while others emphasize practical measurement limitations. The discussion remains unresolved regarding the applicability of theoretical models in extreme scenarios.

Contextual Notes

Limitations include the inability to isolate gravitational influences in experimental settings and the challenges of applying mathematical models to real-world conditions, particularly at cosmological scales.

NODARman
Messages
57
Reaction score
13
TL;DR
.
Hi, mathematically in the F = GMm/r^2 equation r can be very close to infinity (or the size of the universe), but gravitational force always will be some number.
But how is that in the real world? Let's say we have a perfectly empty universe but only with two sun-like stars. If they are away from each other like 45 billion light years, then is their gravitational force still some number or 0?
I took a zero because I'm wondering if space has rubber-like physics. 2D rubber plane with x, y geometrical dimensions and z gravity. If its area is huge (like millions of kilometers ^2), then a small metal ball cannot deform this stretched elastic thing thousands of kilometers away, right? (or it can but it will approach zero?)
If you know what I mean...
Thanks.
 
Physics news on Phys.org
The reach of gravity is infinite in both Newtonian and relativistic gravity, so its effect is always non-zero.

Don't try to reason from a rubber sheet model - it is (at best) illustrative of some situations, but is not remotely rigorous. It would be like trying to deduce how a steam train works by looking at a child's wooden toy.
 
  • Like
Likes   Reactions: vanhees71, topsquark, 256bits and 3 others
NODARman said:
TL;DR Summary: .

Hi, mathematically in the F = GMm/r^2 equation r can be very close to infinity (or the size of the universe), but gravitational force always will be some number.
But how is that in the real world?
The equation of Newtonian gravity you quote is a mathematical model. We can test it in the real universe to some extent. But, there are limits to the experimental data we can collect. For example, there are always multiple sources of gravity and we cannot empty the region of space around the Earth or a star to test the theory beyond what nature allows us to. All we can say is that the equation holds to the extent that we have been able to test it. Moreover, on the largest scales we have an expanding universe and we need GR to model that.

Note that there is no such thing as "close to infinity". We can only say that ##r## is large compared to other factors.
 
  • Like
Likes   Reactions: Vanadium 50, vanhees71, topsquark and 1 other person
NODARman said:
... can be very close to infinity
To expand slightly on what Perok pointed out (because this is a concept that throws people when they're new to it) here's the problem. If you take the largest number that has ever been written down, in whatever exotic form so that it huge beyond belief, the distance from that number to infinity is still ... infinity. So, you aren't any closer than you were at zero.
 
  • Like
Likes   Reactions: vanhees71, NODARman, topsquark and 1 other person
NODARman said:
If they are away from each other like 45 billion light years, then is their gravitational force still some number or 0?
Many things in physics and engineering can be negligibly small. Theory may predict a small nonzero value, but that doesn't mean it can be measured, because measuring instruments have limitations.
 
  • Like
Likes   Reactions: vanhees71, topsquark and NODARman
In your model you should always consider for which values of your parameters the model is still valid. Physicists often do that implicitly. In quantum field theories this question becomes hugely important due to renormalization issues, but already in Newtonian physics this issue plays a role.
 
  • Like
Likes   Reactions: vanhees71

Similar threads

  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 2 ·
Replies
2
Views
1K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 16 ·
Replies
16
Views
2K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 11 ·
Replies
11
Views
3K
  • · Replies 10 ·
Replies
10
Views
2K