Special Relativity and Relative motion

In summary, when the two spaceships collide, the velocity of the spaceship 2 to the frame reference of the spaceship 1 is the same as the velocity of the spaceship 1 to the frame reference of the spaceship 2.
  • #1
olga11
30
0
1. Homework Statement

An observer on Earth sees two spaceships moving in opposite directions and finally they collide. At t=0 the observer on Earth says that the spaceship 1 which moves to the right with Ua=0.8c is at the point A and the spaceship 2 which moves to the left with Ub=0.6c is at the point B. The distance AB=L=4,2.10^8 m.
When do the two spaceships collide to the Earth frame of reference?
What is the velocity of the spaceship 2 to the frame reference of the spaceship 1?
What is the velocity of the spaceship 1 to the frame reference of the spaceship 2?
When does the collision happen to the frame reference of the spaceship 1 and to the frame reference of the spaceship 2?

2. Homework Equations



3. The Attempt at a Solution

Let D be the point of the collision and AD=x, so DB=L-x
The velocity is constant.
spaceship 1: AD=x=0,8c.t
spaceship 1: DB=L-x=0,6c.t
By addition
L=AD+DB
L=(0,8c+0,6c).t
t=4,2.10^8/(1,4.3.10^8)
t=1sec
Is it ok so far?
 
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  • #2
So far, correct.
 
  • #3
The velocity of the spaceship 2 to the frame reference of the spaceship 1 is the same as the velocity of the spaceship 1 to the frame reference of the spaceship 2.
 
  • #4
Numerically, yes. Opp signs because in opp directions. But that shouldn't bother you.
 
  • #5
Using Lorentz transformations

0,8c=(U21-0,6c)/(1-U21.0,6c/c^2)

U21=1,4c/1,48

Correct?
 
  • #6
When does the collision happen to the frame reference of the spaceship 1 and to the frame reference of the spaceship 2?

Now we must use Lorentz transformation for the length?
 
  • #7
olga11 said:
Using Lorentz transformations

0,8c=(U21-0,6c)/(1-U21.0,6c/c^2)

U21=1,4c/1,48

Correct?

(Is your keyboard very old, so you can't tell the , from the .? Just kidding...)

Yes. You could have got it also by (0.8+0.6)c/(1+0.8*0.6).
 
  • #8
olga11 said:
When does the collision happen to the frame reference of the spaceship 1 and to the frame reference of the spaceship 2?

Now we must use Lorentz transformation for the length?

The question is "when", not where. So, use the formula for time.
 
  • #9
Thank you very much for your time.
 

1. What is special relativity?

Special relativity is a theory developed by Albert Einstein that explains how space and time are relative to the observer's perspective. It states that the laws of physics are the same for all observers in uniform motion and that the speed of light in a vacuum is constant.

2. What is the difference between special relativity and general relativity?

Special relativity deals with the effects of relative motion on space and time, while general relativity includes the effects of gravity on the fabric of space-time. Special relativity is applicable in all inertial reference frames, while general relativity extends to non-inertial frames as well.

3. How does special relativity explain time dilation?

According to special relativity, time is relative to the observer's frame of reference. This means that time can appear to pass at different rates for different observers depending on their relative motion. This effect is known as time dilation, where time appears to slow down for objects traveling at high speeds.

4. Can special relativity explain the twin paradox?

Yes, special relativity can explain the twin paradox. This paradox involves one twin traveling at high speed in space while the other remains on Earth. When the traveling twin returns, they will have aged less than the twin on Earth due to time dilation. This is because the traveling twin experienced time passing slower due to their high speed.

5. How does special relativity affect our understanding of space and time?

Special relativity has revolutionized our understanding of space and time by showing that they are not absolute but are relative to the observer's frame of reference. It has also led to the famous equation E=mc^2, which explains the relationship between mass and energy and has had significant implications in fields such as nuclear energy and particle physics.

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