Rocket moving away from the Earth

Click For Summary
SUMMARY

The forum discussion centers on the kinematics of a rocket moving away from Earth and the implications of special relativity on signal transmission between the rocket and Earth. Key equations include the time intervals for signals reaching the rocket and returning to Earth, specifically ##t_4 = T## and ##t_5 = T + \Delta T##. The distance calculations involve the proper length ##l_0## and the gamma factor for time dilation and length contraction. The final derived formula for the distance of the rocket when the signal returns to Earth is ##d = \frac{(c+v)T}{2}##.

PREREQUISITES
  • Understanding of special relativity concepts, including time dilation and length contraction.
  • Familiarity with kinematic equations and their application in relativistic contexts.
  • Knowledge of the gamma factor, defined as ##\gamma = \frac{1}{\sqrt{1 - v^2/c^2}}##.
  • Basic grasp of signal transmission and reflection in physics.
NEXT STEPS
  • Study the derivation and implications of the Lorentz transformations in special relativity.
  • Explore the concept of simultaneity in different reference frames.
  • Learn about the Doppler effect in the context of light signals from moving sources.
  • Investigate practical applications of special relativity in modern physics, such as GPS technology.
USEFUL FOR

Students of physics, particularly those studying special relativity, aerospace engineers, and anyone interested in the kinematics of moving objects in relation to signal transmission.

Physics news on Phys.org
  • #32
Frostman said:
- I know the proper length ##l_0##.
- I know that the time interval between the return of the first and second signal is ##\Delta T##.
- I know that the first signal comes back to Earth after a time of ##T##.
- I know that the second signal comes back to Earth after a time of ##T + \Delta T##.
- While the reflection time interval is equal to ##\frac{\Delta T}2##
- The light signal obviously moves at speed ##1##.

For the contraction of the lengths we have that the Earth measures:

##l = \frac{l_0}{\gamma}=l_0 \sqrt{1-v^2}##

All of this is fine. And the information above is already enough for you to answer the first part of the question--how far the rocket (more precisely, the rear end of the rocket, where the mirror that reflects the first signal is) is from Earth when the first signal arrives (at the mirror on the rear end of the rocket). There's not even any calculation involved; one of the specific quantities you list in the above is the answer to the question (given the units you have chosen, in which ##c = 1##, which are the units I would choose as well).

Frostman said:
I have to find ##l##.

No, you don't, you just gave a formula for it above.

What you need to find is a formula for ##\Delta T## in terms of other quantities, including ##v##. That will allow you to answer the second part of the question, which is, what is ##v##.

Frostman said:
The interval between the two signals reflections is ##\frac{\Delta T} 2##.

Yes, this is correct (assuming that by "interval" you mean "time interval in the Earth frame"). What does this tell you about the distance between the two reflection events, in the Earth frame?

Frostman said:
Is it correct to use the distance traveled by the rocket in this time interval as a length?

A length of what? If you mean a length of the rocket, no, of course not.

Frostman said:
Or is it just a measure of how far the rocket has moved and has nothing to do with the length of the rocket according to earth?

Yes. However, that does not mean the length of the rocket has nothing to do with the problem. You are forgetting to take into account that the first signal reflects off a mirror at the rear of the rocket, while the second signal reflects off a mirror at the front of the rocket. That means the total distance, in the Earth frame, between the two reflection events is made up of two parts, one involving the motion of the rocket and one involving the length of the rocket. Can you see what the two parts are?
 
  • Like
Likes   Reactions: Frostman and Steve4Physics
  • #33
It occurs to me that for the first part they might be asking where the rocket is when it receives the first signal. In which case it's simply ##(c)\frac{T}{2}## and not ##(c+v)\frac{T}{2}##.

Then the second part calculates its speed at that time. And you have the rocket's position and speed at time ##T/2##.
 
  • Like
Likes   Reactions: Frostman
  • #34
PeroK said:
It occurs to me that for the first part they might be asking where the rocket is when it receives the first signal.

That's how I was reading it. How else would you interpret "determine the rocket's distance from Earth at the moment of receiving the first signal"?

PeroK said:
Then the second part calculates its speed at that time.

The rocket's speed is stated to be constant, so any calculation of its speed tells us its speed at any time we like. Knowledge of ##\Delta T## enables us to calculate the average speed between the first and second signal reflection, which is sufficient to answer the second part.
 
  • Like
Likes   Reactions: Frostman
  • #35
PeterDonis said:
That's how I was reading it. How else would you interpret "determine the rocket's distance from Earth at the moment of receiving the first signal"?
When the signal is received back on Earth. Originally, I didn't think light bouncing off a mirror was a signal being received by the ship. In any case, estimating the speed is the key part of the question.
 
  • Like
Likes   Reactions: Frostman
  • #36
PeroK said:
When the signal is received back on Earth. Originally, I didn't think light bouncing off a mirror was a signal being received by the ship.

Ah, I see. Well, one can always calculate both to be covered either way. :wink:
 
  • Like
Likes   Reactions: Frostman
  • #37
The OP seems to have put effort in. Much of the explanation has been given, but is 'scattered'. So I’m taking a bit of a liberty and posting this, hoping it will help and that it's OK with @PeroK and @PeterDonis.

Q1.

It takes time ##T## for the light to return from the rear mirror: ##\frac T 2## traveling outwards and ##\frac T 2## returning.
If the rear mirror is a distance ##d## from the source at the moment of reflection, this means: ##d = speed * time = c\frac T 2##

This is the same calculation as used in elementary (sound) echo problems. It has nothing to do with relativity.

Q2.

Let P be the position of the rear mirror at the moment it reflects.

##\Delta T## is the time for the light to travel from P to the front mirror and back to P: ##\frac {\Delta T} 2## traveling outwards and ##\frac {\Delta T} 2## returning.

Distance moved by front mirror in time ##\frac {\Delta T} 2## is ##v \frac {\Delta T} 2##.

If ##l## is the (contracted) length (distance between mirrors as observed from earth) then in time ##\frac {\Delta T} 2## the light covers a total distance ##l + v\frac {\Delta T} 2##

Also in time ##\frac {\Delta T} 2## we know light covers a distance ##c\frac {\Delta T} 2##, giving the equation:

##c\frac {\Delta T} 2 = l + v\frac {\Delta T} 2##

No relativity needed up to this point! If we replace ##l## with ##l_0 \sqrt{1-{(\frac v c})^2}## we now have an equation from which v can be found.

Edit - unclear wording improved.
 
Last edited:
  • Like
Likes   Reactions: Frostman and PeroK
  • #38
Comment 1: you didn't put in equations in the "relevant equations" part of the template. That was a mistake.

Comment 2: you don't seem to have a plan. You seem to be calculating random things hoping one will be the answer. This strategy will not get you successfully through a PhD program.

I suggest you start over. Write down the plan on how you will solve this. Write down the equations you need to execute this plan. Then execute the plan.
 
  • Like
Likes   Reactions: Frostman
  • #39
I understand the problem, I find it hard to frame the situation.
For example, I didn't really get to the fact that yes, ##c \frac{\Delta T} {2}## is the distance traveled by the light, but it's not the length of the rocket, it's the length of the rocket plus the distance traveled by the rocket in that time interval.
The exercise itself is as simple as it is banal. In the end it was a question of remembering the equations of uniform motion and then understanding what those times actually represented.
I apologize to all of you, especially @PeroK for wasting your time.
In the next few times I will try to focus more on the knowledge I have available and to try, as far as I can, to understand the text better.
 
  • Like
Likes   Reactions: Tom.G, phinds, berkeman and 3 others

Similar threads

  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 4 ·
Replies
4
Views
2K
Replies
6
Views
2K
  • · Replies 25 ·
Replies
25
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 2 ·
Replies
2
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
Replies
3
Views
2K