Length contraction near the speed of light

In summary, an astronaut traveling at close to the speed of light could reach the far edge of the Milky Way within their lifetime. Time would pass slowly for the astronaut as they moved across the galaxy, and the length of the galaxy would appear to contract in their direction of motion. However, from the astronaut's perspective, the distance would still be relatively short. The number of stars in the galaxy would not change, but they would appear contracted as well. This raises questions about the laws of physics and how they would apply in a moving system. For example, the size of electron orbits around atoms may appear different for the astronaut compared to someone on Earth.
  • #1
chrispegg
3
0
It is my understanding that an astronaut could get from Earth to the far edge of the Milky Way within the length of a human lifetime if she were traveling close enough to the speed of light. From earth’s perspective, time would pass very slowly for her as she moved across the galaxy. From the spaceship’s perspective, the length of the galaxy would contract in her direction of motion with respect to the galaxy.

Therefore, it seems to me that, from the astronaut’s perspective, the distance between Earth and the far edge of the galaxy would be very short (comparatively speaking) in her direction of motion. But, of course, the number of stars in the Milky Way that she will pass on her journey will not change.

How do all those stars fit in such a small space?
 
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  • #2
chrispegg said:
How do all those stars fit in such a small space?
They are also contracted.
 
  • #3
Yes, but hasn't all of physics changed from the spaceship's perspective? How, for instance, do all the atoms of a contracted star fit within such a short distance without collapsing into a black hole?

Does the astronaut have to teach her child a different kind of physics regarding the size of an electron orbit around a hydrogen atom, etc?
 
  • #4
chrispegg said:
Yes, but hasn't all of physics changed from the spaceship's perspective? How, for instance, do all the atoms of a contracted star fit within such a short distance without collapsing into a black hole?

Does the astronaut have to teach her child a different kind of physics regarding the size of an electron orbit around a hydrogen atom, etc?
Many laws of physics, such as the one that you hint at, are formulated for systems that are in rest; that allows for the simplest formulation. They should not be applied to moving systems, instead the moving system description must be transformed to that of a rest frame. This is to a lesser extent already the case in classical (Newtonian) mechanics: the orbits of planets in a moving solar system are not ellipses but spirals. And of course, this problem does not occur for the electron orbits of the spaceship's atoms.
 

What is length contraction near the speed of light?

Length contraction is a phenomenon in which an object's length appears to decrease when it is in motion at speeds close to the speed of light.

How does length contraction occur?

Length contraction occurs due to the effects of special relativity, which states that the laws of physics are the same for all observers in uniform motion. As an object approaches the speed of light, its relative motion causes its length to decrease in the direction of motion.

What is the equation for calculating length contraction?

The equation for calculating length contraction is L = L0 * √(1 - v^2/c^2), where L is the contracted length, L0 is the object's rest length, v is its velocity, and c is the speed of light.

At what speed does length contraction become noticeable?

Length contraction becomes noticeable at speeds close to the speed of light, which is approximately 299,792,458 meters per second. However, the effects of length contraction are only significant at speeds that are a significant fraction of the speed of light.

What are the implications of length contraction in our daily lives?

Length contraction is only noticeable at speeds close to the speed of light, which is much faster than anything we experience in our daily lives. Therefore, its effects are not significant in our everyday experiences. However, it is a fundamental principle in physics and plays a crucial role in understanding the behavior of objects at high speeds.

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