Perpendicular relative velocities

In summary, the conversation discusses different approaches to finding the wavelength of radiation emitted by rocket B as seen by rocket A, which is moving at .75c in a northerly direction relative to an origin. The first approach is incorrect, while the second involves using Lorentz transformation and four-vectors to calculate the emission direction in A's reference frame. The variables used include v^0 and v^A for the origin's and A's reference frames, respectively, and V_A for the speed of rocket A.
  • #1
moogull
86
0

Homework Statement



Rocket A moves with speed .75c in a northerly direction relative to an origin. Rocket B moves west (relative to that origin) with speed .4c. As B moves, it emits radiation with a wavelength 100nm normal to its line of motion, in the northerly direction. What is the wavelength of the radiation as seen by A?


Homework Equations



Doppler shift equations
Velocity addition formulas

The Attempt at a Solution



So far I have two different approaches to a solution, the first approach finds the wavelength of the radiation as seen by a person at the origin (which is redshifted) because the source is moving away at .4c. Then use that wavelength to find the wavelength as seen by a person moving away at .75c (to represent the rocket A). I'm not so sure about this solution...

The second idea I had was to find the relative velocity of B as seen by A (since it would be a right triangle) and using those to find the angle between the light source and the observer. However, I am unsure how to find the separate components of the relative velocity. Do I keep the .75c speed in one direction and uy = uy' /(gamma(1-ux*v/c^2) to find the other direction, if that is so I have no idea what the relative velocity would be... This method is really tripping me up and I think it is the correct way. Could someone help me get on the right track?
All incite is appreciated
 
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  • #2
The first way is incorrect. The observer should be at A position, not at the origin.

The second way is correct, but you will have to recalculate the emission direction.

I think the simplest way is to use Lorentz transformation to find photon's momentum-energy four-vector:
[tex] p^i = \left( \frac{h\nu}{c}, hk_x, hk_y, hk_z \right) [/tex]
in origin's reference frame and then find it in A rocket's reference frame.
 
  • #3
Darn, I am unfamiliar with this energy momentum four vector, my professor has just given us the velocity addition formulas and a few doppler shift formulas. Is it possible to find the "resultant" velocity of ship B according to ship A?
 
  • #4
Yes, it is.

The corresponding formulas are
[tex]
v^A_x = \frac{v^0_x - V_A}{1-(v^0_x V_A)/c^2}
[/tex]
[tex]
v^A_y = \frac{v^0_y\sqrt{1-V_A^2/c^2}}{1-(v^0_x V_A)/c^2}
[/tex]

The "0" superscript means the origin's reference frame (RF) and "A" means A rocket's RF.

Remember that emission direction in RF A and RF B is different.

In fact, four-vectors is another way to write these formulas. I like it because it's easier for me to remember one matrix than four equations.
 
  • #5
O, that does sound useful, only had minor exposure to matrices so far but I'm building my base knowledge. Another question: for VsubA do I use the speed of rocket ship A? I'm unsure as to what variable represents what speed. Sorry to be such a noob :/
 
  • #6
Yes, V_A is the speed of rocket A.
 
  • #7
Thank you very much Maxim, I think I've got it, have a good one
 

Related to Perpendicular relative velocities

1. What is the definition of perpendicular relative velocities?

Perpendicular relative velocities refer to the velocities of two objects moving in different directions relative to each other, with one velocity being perpendicular to the other. This means that the two objects are moving at right angles to each other.

2. How do you calculate the perpendicular relative velocity?

The perpendicular relative velocity can be calculated using vector addition. This involves finding the vector components of each object's velocity and adding them together to determine the resultant velocity. The magnitude of the resultant velocity is the perpendicular relative velocity.

3. What is the significance of perpendicular relative velocities in physics?

Perpendicular relative velocities are important in understanding the motion of objects and their interactions in physics. They can help determine the direction and magnitude of forces acting between objects, and are essential in analyzing motion in two or three dimensions.

4. Can perpendicular relative velocities ever be equal?

No, perpendicular relative velocities can never be equal because they are always moving in different directions. If they were equal, they would not be perpendicular to each other. However, two objects can have equal perpendicular components of their velocities, resulting in a perpendicular relative velocity of zero.

5. How does the angle between the two velocities affect the perpendicular relative velocity?

The angle between the two velocities affects the magnitude of the perpendicular relative velocity. The smaller the angle between the velocities, the larger the perpendicular relative velocity will be. When the angle is 90 degrees, the perpendicular relative velocity will be the sum of the two individual velocities.

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