friendbobbiny said:
Why is this true? That simultaneity holds for all frames given those conditions (for distance and time) in one frame?
When two events happen at the exactly at the same place and at the same time, as measured in any given frame, those two events are really just one, single event. And it will be observed as a single event in all frames. [Edit: I must re-iterate though that this only applies to events that share the same point in both space and in time. It does not apply to events in the same place but at different times, nor does it apply to events measured to be "simultaneous" in a given frame, but at different points in space. It only applies when events share points in
both space
and time, in any given frame of reference.]
Transforming from one frame of reference to another only involves transforming spacetime
coordinates, but does not alter the spacetime events themselves. If two events share the same spacetime coordinates in one frame of reference, they share the same coordinates in any frame of reference. (The numerical value of the shared coordinates will be different one one frame than the value of the shared coordinates of another frame; what I mean to say is that the events will still be shared, no matter what the frame. If they are shared in one frame, then they are shared in all frames.)
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Allow me to introduce a new tool that might be helpful.
If you continue to learn about special relativity, there is tool you will learn about called a "spacetime diagram," if you haven't learned about it already. Spacetime diagrams are very useful and insightful.
The general idea is that you plot time on the vertical axis and space on the horizontal one. This corresponds to some particular, inertial frame of reference.
Every point on the graph represents an "event." You can transition between frames, not by altering any of the events, but rather by altering the coordinates: You change the orientations of the axes, without altering the events at all.
The math is a little different from Euclidean math though. The length between two points on angled line is not \sqrt{ \left( \Delta x \right)^2 + \left( c \Delta t \right)^2} as you might expect, but rather it's \sqrt{ \left( \Delta x \right)^2 - \left( c \Delta t \right)^2} for space-like separations and \sqrt{ -\left( \Delta x \right)^2 + \left( c \Delta t \right)^2} for time-like separations. Also, hyperbolic functions replace trigonometric ones. But that's all in the details. One neat thing about them is that you can use spacetime diagrams to do Lorentz transformations geometrically (among other uses).
The thing I'm trying to point out with this is that as you change from one frame to another, none of the events on the paper are altered. The only thing that changes is the coordinate system that indicates relative distance and time intervals.
If two events share the same spacetime coordinates (both time and space) in a given frame, they correspond to a single point on the spacetime diagram. When changing frames, the points (i.e., events) are not modified. Only the diagram's axes are modified. But since the points are not modified, a single point in one frame will remain a single point in all frames.