Hubble's Law and Acceleration: Are Distant Objects Accelerating Away from Us?

  • Thread starter Mechanic
  • Start date
  • Tags
    Hubble
In summary, Hubble's law states that the velocity of distant objects increases with distance according to the equation v=Hr. This suggests that as distant objects move farther away, they recede at a faster rate. This can be seen as acceleration, with a corresponding equation of dv/dt=H dr/dt + r dH/dt=Hv=(H^2)r. However, it has been observed that H(t) has been declining and is expected to continue to decline, leading to a slowing of this acceleration. It is not expected to ever increase, only to gradually level out to a constant. The projected percentage growth rate of large-scale distances is 1/173 of one percent per million years according to the Lambda
  • #1
Mechanic
51
1
Hubble’s law tells us that the velocity of distant objects increases with distance as v = Hr. Does this mean that the farther a distant object gets the more rapidly that object will recede away from us? That is, are these distant objects accelerating away from us? Can we say
v = Hr, and so Acceleration = dv/dt =H dr/dt + r dH/dt = Hv = (H^2)r for constant H? Has such an acceleration been observed/measured?

Thanks
 
Astronomy news on Phys.org
  • #2
H(t) has been declining since the first few seconds of expansion (as far as we know) and according to best fit model matching observations (LambdaCDM, the standard one people use) has been declining for past billions of years and WILL CONTINUE to decline *but at a slowing rate*. This slowing of the rate that H(t) is declining corresponds to what they call "acceleration" or "dark energy effect"or "cosmological constant effect".

It is not expected to make H(t) ever increase, only slow decline and gradually makeH(t) essentially level outy to be constant. Then your equation is right! Constant H(t) would lead to exponential expansion. i.e. fixed percentage growth

The projected percentage growth rate of large-scale distances (not expected to affect galaxy scale distances) according to LCDM model is 1/173 of one percent per million years.

You might take a look at the tabular calculator that one of PF members made that shows past and future history. It will show the change o over time of 1/H or c/H (which grows as H decreases)

It is "Lightcone" calculator link in my sig. click on it, you can adjust the parameters at will.

You can get it to show the acceleration in distance growth that started around year 7 billion. but that takes a little work, so ask questions if you want on how to use it.
 
  • #3
Thanks for the info. It will take a while to fully digest...but the fact the distant objects are moving from us at v=Hr and ACCELERATING away from us as/if H(t) is constant is very interesting.
 

1. What is Hubble velocity/acceleration?

Hubble velocity or Hubble flow is the apparent velocity at which galaxies are moving away from us due to the expansion of the universe. Hubble acceleration, on the other hand, refers to the change in this velocity over time.

2. How is Hubble velocity/acceleration measured?

Hubble velocity and acceleration are measured using a unit called the Hubble constant, which represents the rate of expansion of the universe. This constant is determined by measuring the redshift of light from distant galaxies.

3. What is the significance of Hubble velocity/acceleration?

Hubble velocity and acceleration help us understand the large-scale structure and evolution of the universe. They also provide evidence for the theory of the Big Bang and the ongoing expansion of the universe.

4. How does Hubble velocity/acceleration affect the motion of galaxies?

Hubble velocity and acceleration cause galaxies to move away from each other at an increasing rate. This is due to the expansion of the universe, which is pushing galaxies further apart.

5. Can Hubble velocity/acceleration be observed in our own galaxy?

Yes, the Hubble velocity and acceleration can be observed in our own galaxy, the Milky Way. However, it is difficult to measure due to the relatively small distances involved compared to the vast distances between galaxies.

Similar threads

  • Astronomy and Astrophysics
Replies
13
Views
2K
  • Astronomy and Astrophysics
Replies
5
Views
2K
  • Special and General Relativity
Replies
15
Views
1K
Replies
35
Views
1K
  • Special and General Relativity
2
Replies
40
Views
3K
Replies
6
Views
4K
Replies
5
Views
1K
  • Introductory Physics Homework Help
2
Replies
42
Views
3K
Replies
6
Views
707
Replies
3
Views
2K
Back
Top