PhMichael
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There's something about the lorentz transformations which is somewhat confusing to me, and that is how to treat the "x" coordinate. Supposing I have some spaceship which is moving from Earth to some other planet located at a distance "D" (from earth) with a velocity v. Now, the spacetime coordinates of the events "1. leaving earth" and "2. reaching the planet" are (the spaceship frame is {S'} and that of Earth is {S} ) :
Leaving earth:
(x_{1},t_{1})=(x'_{1},t'_{1})=(0,0)
Reaching the planet:
(x_{2},t_{2})=(D, \frac{D}{v} )
(x'_{2},t'_{2})=(0 , \gamma (t_{2} - (v/c^{2})x_{2})=(0 , \gamma (t_{2} - (v/c^{2})D)
Now comes the confusing point which is how to treat x_{3} which corresponds to the event of returning back to Earth in the Earth's frame. (in the spaceship frame it is x'_{3} = 0 )
The Lorentz transformations relates coordinates and not distances so x_{3} = 0 because the spaceship returns to the origin of Earth and t_{3} = \frac{2D}{v}. However, as I have seen in my notes:
x_{3} = 2D
, that is, the distance that this spaceship travels is what is accounted for and not its coordinate.
Can anyone clear this point for me?
Leaving earth:
(x_{1},t_{1})=(x'_{1},t'_{1})=(0,0)
Reaching the planet:
(x_{2},t_{2})=(D, \frac{D}{v} )
(x'_{2},t'_{2})=(0 , \gamma (t_{2} - (v/c^{2})x_{2})=(0 , \gamma (t_{2} - (v/c^{2})D)
Now comes the confusing point which is how to treat x_{3} which corresponds to the event of returning back to Earth in the Earth's frame. (in the spaceship frame it is x'_{3} = 0 )
The Lorentz transformations relates coordinates and not distances so x_{3} = 0 because the spaceship returns to the origin of Earth and t_{3} = \frac{2D}{v}. However, as I have seen in my notes:
x_{3} = 2D
, that is, the distance that this spaceship travels is what is accounted for and not its coordinate.
Can anyone clear this point for me?
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