A thought on the expansion of the Universe

In summary: However, if we have more information about the atmosphere, we might be able to say that there is a 50% chance of frost.In summary, galaxies are moving away from us faster than galaxies that are closer to us, but we can also look back in time and observe galaxies that are further back in space. We know this because of the red shift of the light from these galaxies.
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Igottaknow
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One thing that has always puzzled me is that the farther we look out into the universe we see that galaxies are moving away from us faster than galaxies that are closer to us, but also the farther we look out into space the farther back in time we are observing.

I have trouble understanding this since we know that what we are observing when we view a galaxy 4 billion light years away is what was happening 4 billion years ago. What is it about that light that we can say for certain that that galaxy is moving away from us at any specific rate as it is in relation to us now?

I do understand that it is is because of the red shift of this 4 billion year old light and the idea of the Doppler effect of that light that we have determined that galaxy's rate of movement but...how do we know for certain anything about what is happening with that galaxy right now in that region of space?

I guess i am trying to understand how we can determine for certain any thing about what we observe in the universe not being anything other than what was happening at the time the light left that object.
 
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If something was moving away from us at half the speed of light 4 Billion years ago, we can look at what was around it and determine what kind of gravitational pull is being applied to it. When can then determine whether it is going to continue moving away at the same speed, slow down but continue moving away, or slow down and reverse direction.

... and it's all going to continue moving away.
 
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We can't say with certainty what will have happened to a distant galaxy which we are seeing as it was billions of years ago.
There could be unforeseeable events due to gravitational interactions with other galaxies.
However we can make reasonable predictions from models and rule out some possibilities, such as that galaxy spontaneously disintegrates.
It's the same in principal as a weather forecast; we can say that given the present data rain can be expected tomorrow and there is no chance at all of frost.
 
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1. What is the theory of the expansion of the Universe?

The theory of the expansion of the Universe is the widely accepted scientific explanation for the continuous and ongoing increase in the distance between galaxies. It suggests that the entire Universe is expanding, with galaxies moving away from each other at an accelerating rate.

2. How was the theory of the expansion of the Universe discovered?

The theory of the expansion of the Universe was first proposed by Belgian astronomer Georges Lemaître in 1927. However, the discovery of the Cosmic Microwave Background Radiation in 1964 provided strong evidence for the theory and solidified its acceptance among the scientific community.

3. What is dark energy and how does it relate to the expansion of the Universe?

Dark energy is a mysterious force that is believed to be responsible for the acceleration of the expansion of the Universe. It is thought to make up about 68% of the total energy in the Universe and its presence is necessary to explain the observed rate of expansion.

4. Is the expansion of the Universe uniform?

No, the expansion of the Universe is not uniform. This means that different regions of the Universe are expanding at different rates. This non-uniform expansion is known as the Hubble flow and is caused by the distribution of matter and energy in the Universe.

5. How does the expansion of the Universe affect objects within it?

The expansion of the Universe does not directly affect objects within it. This is because the expansion is happening at a cosmological level and on a much larger scale than individual objects. However, the ongoing expansion of the Universe will eventually result in the separation of galaxies and the eventual cooling and darkening of the Universe.

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