Transformation equation of velocity contradicts stellar aberration?

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Discussion Overview

The discussion revolves around the transformation of velocities in different reference frames, particularly in the context of stellar aberration and special relativity. Participants explore how light from distant stars behaves when observed from a moving frame compared to a stationary frame, questioning the implications of velocity transformation equations.

Discussion Character

  • Technical explanation, Conceptual clarification, Debate/contested

Main Points Raised

  • One participant describes a scenario involving light from the North Star and another star, questioning whether two perpendicular vectors remain perpendicular when changing reference frames.
  • Another participant suggests that the light from the North Star should gain an x component due to the observer's motion, expressing uncertainty about the transformation equations used.
  • Clarification is provided regarding the meaning of u and u', identifying them as velocities in different frames.
  • One participant asserts that transforming the velocity of the North Star will reveal an x component in the moving frame, indicating a change in orthogonality.
  • A participant challenges the understanding of special relativity, implying that the transformation may not yield the expected results for non-parallel velocities.
  • Another participant acknowledges a mistake in their previous reasoning after receiving feedback, indicating a shift in understanding.
  • Discussion includes the idea that in both moving frames, there must be a non-orthogonal velocity component between the two rays of light.
  • One participant notes a correction regarding the velocity transformation, mentioning the need for a factor of 1/gamma in the equations.

Areas of Agreement / Disagreement

Participants express differing views on the implications of velocity transformations, particularly regarding the orthogonality of light paths in different frames. There is no consensus on the correct interpretation of the transformation equations or the behavior of light in this context.

Contextual Notes

Some participants indicate limitations in their understanding of special relativity, which may affect their interpretations of the transformation equations and the resulting implications for light propagation.

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Let S be the frame where the Sun is at rest. Imagine light from the North Star reaches the centre of the Sun, and let's define the equatorial plane as the plane that is perpendicular to this light and cuts the Sun into two hemisphere.

Suppose a distant star A is on this equatorial plane and its light also reaches the centre of the Sun. Let the direction of the propagation of this light be our x axis. And let our y-axis be pointing in the direction of the North Star.

In other words, the light from star A is traveling in the positive x direction, while that from the North Star is traveling in the negative y direction.

Let S' be the frame that is moving with respect to S in the positive x direction at velocity v.

By the transformation equation of velocity,

##u_x^\prime=\frac{u_x-v}{1-u_xv/c^2}## , ##u_y^\prime=\frac{u_y\sqrt{1-v^2/c^2}}{1-u_xv/c^2}## , ##u_z^\prime=\frac{u_z\sqrt{1-v^2/c^2}}{1-u_xv/c^2}##

the light from the North Star and that from star A are still traveling in the negative y direction (or y', to be precise) and in the positive x direction (or x'), respectively, to an observer in S'.

This contradicts the observation of stellar aberration, where the two velocities are not perpendicular in S'.

What did I miss?

Are two perpendicular vectors still perpendicular when we change reference frames?
 
Last edited:
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Conceptually, I would think that they would not be perpendicular in S'. The light from the north star should gain a x component due to the observers velocity in the x direction. I'm also not sure what you're doing with the transformation equations. What is u the velocity of?
 
u and u' are the velocities in S and S', respectively.

##u_{North\ Star}##, velocity of light from the North Star in frame S = ##\begin{pmatrix}u_x\\u_y\\u_z\end{pmatrix}## = ##\begin{pmatrix}0\\-c\\0\end{pmatrix}##
 
Ok, so transform ##u_{North Star}## to ##u_{North Star}'## and you'll see that in one frame, u', you have an x component from the orthogonality of the two velocities.
 
No, it does not. Have you learned special relativity before?
 
-.-
##\left ( \begin{array}{c}
0 \\
-c \\
0 \\
\end{array} \right ) ##
##
\left ( \begin{array}{c}
v \\
0 \\
0 \\
\end{array} \right ) ##
##u'=\frac{u-v}{ 1-\frac{uv}{c^2}}
=\frac{
\left ( \begin{array}{c}
0 \\
-c \\
0 \\
\end{array} \right ) -
\left ( \begin{array}{c}
v \\
0 \\
0 \\
\end{array} \right )}{1-\frac{uv}{c^2}}
##
What you are trying to do is set up the transforms for when the velocity of the north star is along the x-axis (parallel to the velocity).

Also, no, I haven't learned SR. I have, however, studied it. Once I learn it, I will quit studying it.
 
Oh yes, you are right! Now, I see the mistake. Thanks!
 
Think about it like this. If these 2 rays of light are going to meet at the center of the sun, then in their respective frames (S' and S'', where S'' has a velocity along the y-axis parallel to the velocity of the north star light coming towards the sun ), there must be a non orthogonal velocity component between the 2 frames in BOTH frames (S' and S'')
 
No problem, but do me a favor, and don't attack people that are trying to help you like that.
 
  • #10
Yes, don't take it to heart.
 
  • #11
BiGyElLoWhAt said:
u&#039;=\frac{u-v}{ 1-\frac{uv}{c^2}}<br /> =\frac{<br /> \left ( \begin{array}{c}<br /> 0 \\<br /> -c \\<br /> 0 \\<br /> \end{array} \right ) -<br /> \left ( \begin{array}{c}<br /> v \\<br /> 0 \\<br /> 0 \\<br /> \end{array} \right )}{1-\frac{uv}{c^2}}
That's not correct for non-parallel velocities. See velocity-addition formula.
 
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  • #12
Ahh, true, I missed a 1/gamma on my v. Regardless, the point is that the velocities have non orthogonal components after you transform out of the S frame to S' or S''.
 

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