This might help...
it's a new update of my desmos "spacetime diagrammer" (
https://www.desmos.com/calculator/nilbye4ecz ) .
The key idea is this...
Short answer:
"space is perpendicular to time"
Slightly longer answer:
"an observer's sense of space [her spaceline] is 'perpendicular' to an observer's sense of time [her worldline]"
One can define "perpendicularity" using a unit circle.
Then, the tangent line to that circle is perpendicular to the radial line.
Refer to the visualization (
https://www.desmos.com/calculator/nilbye4ecz )
The t-axis [to be interpreted as time in the spacetime cases] runs to the right and
the y-axis runs upwards.
You can tune the slopes [to be interpreted as velocities in the spacetime cases] of the [world]lines.
You can tune the choice of circle [to be interpreted as "being one tick after the origin event O" in the spacetime cases].
The black point [event] represents a point you can drag around... representing the point [event] of interest.
The green and red points represents points along the [world]lines, together with the "perpendicular direction" (defined by the chosen type of circle).Consider the
Euclidean case (Set the "E= -1" in the visualization. The metric)
Here's how the green line will assign coordinates.
- Drag the green point so that the associated perpendicular meets the distant black point.
- According to the green line, the distant black point has the same "t"-coordinate [according to green] as the black point.
- Measure the distance (call it "y" according to green) along that perpendicular. (The visualization doesn't show this measurement explicitly, yet. But it conveys the idea.)
The red line will assign coordinates in an analogous way.
In general, the green and red lines will assign different t's and y's... but they will agree that on the value of ##t^2+y^2## (the square distance from O)
Now consider the
special relativity case (set the slider to E= +1).
In general, the green and red lines will assign different t's and y's... but they will agree that on the value of ##t^2-y^2## (the square interval from O)
I encourage you to look at the E=0 case (set the slider to E= 0), which corresponds to
Galilean case.
In general, the green and red lines will assign the
same t's [
absolute time] but different y's...
(they will agree that on the value of ##t^2## (the Galilean square interval from O)).