How the universe looks like at the speed of light

In summary, at close to the speed of light, the universe would still appear relatively the same, but with some optical effects such as rotation, compression, and shifting of wavelengths. There may also be a ring where cosmic microwave background radiation becomes visible, and hard gamma bursts may be visible behind in the forward field of view. However, as the speed approaches c, everything behind will be moved into the forward field of view due to abberation.
  • #1
yoelhalb
69
0
How those the universe physicly looks like close to the speed of light, is it a flat disk or something different. (NOTE I am not asking in measurments accurding to someone that is not traveling but rather how it looks to himself)
 
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  • #2
I've seen a calculation that says everything looks rotated as you approach the speed of light. In other words, if you were passing by a star at close to the speed of light, it wouldn't look like an oval, it would still be round...just rotated compared to what it would be if you were at rest with respect to it. So I'm guessing the universe would still look like it normally does...just take every star and turn it a little bit.
 
  • #3
I think everything would look rather smeared.
 
  • #4
Because of Lorentz contraction, as you approached the speed of light, the universe would be compressed to a single plane, with no distance in the direction that you are traveling, but the same as it was in the other directions.
 
  • #5
Thanks to share this information
 
  • #6
There are two primary optical effects, Doppler shift and abberation. The abberation will cause things that are to your side (in the "stationary" frame) to appear to the front. The Doppler shift will cause things in front of you to be higher wavelengths and things behind you to be lower wavelengths. If you are going fast enough there will be a ring where the cosmic microwave background radiation is shifted into the visible. Inside that ring you will see nothing as everything will have been blueshifted beyond the visible, outside that ring will be a region where the stars have not been blueshifted beyond the visible, but they will be affected by abberation. Looking directly behind yourself you may be able to see hard gamma bursts that have been redshifted into the visible.
 
  • #7
DaleSpam said:
Looking directly behind yourself you may be able to see hard gamma bursts that have been redshifted into the visible.

Except that at nearly c, there is nothing behind you to look at. Abberration moves all images into your forward field of view. There's a good video of optical effects here:

https://www.youtube.com/watch?v=JQnHTKZBTI4
 

FAQ: How the universe looks like at the speed of light

What is the speed of light?

The speed of light is a fundamental constant in physics, denoted as "c". It is approximately 299,792,458 meters per second in a vacuum.

How does the universe look like at the speed of light?

At the speed of light, time and space become relative, and the laws of physics as we know them may no longer apply. It is difficult to imagine or visualize what the universe would look like at this speed.

Can we travel at the speed of light?

According to the theory of relativity, it is impossible for any object with mass to reach or exceed the speed of light. However, scientists are continually exploring ways to travel at high speeds, such as through the use of spacecraft and advanced propulsion systems.

Does the speed of light affect how we see the universe?

Yes, the speed of light plays a crucial role in how we see the universe. Since light takes time to travel, the further an object is from us, the longer it takes for the light from that object to reach our eyes. This means that when we look at objects in the night sky, we are seeing them as they appeared in the past.

What is the cosmic speed limit?

The cosmic speed limit, also known as the speed of light, is the maximum speed at which energy, matter, and information can travel through space. It is a fundamental limit in the universe and is essential in understanding the laws of physics and the nature of our universe.

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