Special Relativity clarification required

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SUMMARY

The discussion centers on a special relativity problem involving two spaceships, each 100 meters long at rest, traveling towards each other at 0.85c relative to Earth. The length contraction formula, L = 1/γ * Lp, results in each ship appearing 53 meters long from Earth's frame. The time for their backs to meet is calculated using t = L/u, yielding 2.1e-7 seconds. The confusion arises from understanding why only one ship's length is considered despite both moving towards each other, which is clarified by focusing on the Earth's frame of reference.

PREREQUISITES
  • Understanding of special relativity concepts, particularly length contraction.
  • Familiarity with the Lorentz factor (γ) and its calculation.
  • Knowledge of relativistic velocity transformation equations.
  • Ability to apply basic kinematic equations in relativistic contexts.
NEXT STEPS
  • Study the derivation and implications of the Lorentz factor (γ) in special relativity.
  • Learn about the relativistic velocity transformation equations in detail.
  • Explore examples of length contraction and time dilation in various frames of reference.
  • Practice solving problems involving multiple objects in relative motion using Earth's frame of reference.
USEFUL FOR

Students studying physics, particularly those focusing on special relativity, as well as educators seeking to clarify concepts related to relativistic motion and reference frames.

PsychonautQQ
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Homework Statement


Two spaceships, each 100m long when measured at rest, travel toward each other, each with a speed of .85c relative to the earth. At time t=0 on earth, the front ends of the ships are next to each other as they just begin to pass each other. At what time on Earth are their backs next to each other?


Homework Equations


L = 1/γ * Lp
t = L/u


The Attempt at a Solution


So the length of each ship from Earth's frame is 1/γ * Lp which comes out to 53 meters, and then apparently the time it takes for their back ends to be together is the time it takes either spaceship to move the length of the spaceship in Earth's frame. So it would be t = L/u which comes out to 2.1e-7 seconds.
The book says this is the correct answer, but I don't understand. Why do you only need to calculate the time it takes for one spaceship to travel the length of a spaceship from Earth's frame? Shouldn't the fact that they are both moving towards each other from Earth's frame mean something?

wtfz
Special relativity is confusing me in general actually... can somebody explain the relativistic velocity transformation equations to me??

ux = (u'x + v) / (1+ (vu'x/c^2))

and yet...

uy = u'y / γ(1+ (vu'x/c^2))

how come the relative velocity of the particle in the x direction effects it's velocity transformation in the y direction? I know it has to do with the fact that the frame S and S' are moving apart from each other in the x direction but I can't quite connect the dots for making sense of this equation, anyone think they can enlighten me?
 
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PsychonautQQ said:
Why do you only need to calculate the time it takes for one spaceship to travel the length of a spaceship from Earth's frame? Shouldn't the fact that they are both moving towards each other from Earth's frame mean something?

A picture in the Earth frame showing the locations of the ships when their front ends are coincident and then when their back ends are coincident should make this clear.

how come the relative velocity of the particle in the x direction effects it's velocity transformation in the y direction? I know it has to do with the fact that the frame S and S' are moving apart from each other in the x direction but I can't quite connect the dots for making sense of this equation, anyone think they can enlighten me?

uy = Δy/Δt and u'y = Δy'/Δt'

Although Δy = Δy', Δt differs from Δt' due to the relative motion of the frames in the x direction. It might help to review the derivation of the velocity transformation equations.
 
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PsychonautQQ said:

Homework Statement


Two spaceships, each 100m long when measured at rest, travel toward each other, each with a speed of .85c relative to the earth. At time t=0 on earth, the front ends of the ships are next to each other as they just begin to pass each other. At what time on Earth are their backs next to each other?


Homework Equations


L = 1/γ * Lp
t = L/u


The Attempt at a Solution


So the length of each ship from Earth's frame is 1/γ * Lp which comes out to 53 meters, and then apparently the time it takes for their back ends to be together is the time it takes either spaceship to move the length of the spaceship in Earth's frame. So it would be t = L/u which comes out to 2.1e-7 seconds.
The book says this is the correct answer, but I don't understand. Why do you only need to calculate the time it takes for one spaceship to travel the length of a spaceship from Earth's frame? Shouldn't the fact that they are both moving towards each other from Earth's frame mean something?

wtfz
Special relativity is confusing me in general actually... can somebody explain the relativistic velocity transformation equations to me??

ux = (u'x + v) / (1+ (vu'x/c^2))

and yet...

uy = u'y / γ(1+ (vu'x/c^2))

how come the relative velocity of the particle in the x direction effects it's velocity transformation in the y direction? I know it has to do with the fact that the frame S and S' are moving apart from each other in the x direction but I can't quite connect the dots for making sense of this equation, anyone think they can enlighten me?

The problem is asking how long it takes the ships to pass each other as reckoned from the Earth's frame of reference. That is why the focus is on the Earth's frame of reference, and not the frames of reference of the two ships. You analyzed the problem flawlessly.
 

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