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add references to "Relativity on Rotated Graph Paper"
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robphy
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To help in "visualizing proper time", here is a spacetime diagram on rotated graph paper.
The key feature in the construction is that the area of the "light-clock diamonds" (marking off the ticks of a wristwatch) are equal in magnitude along different inertial worldlines.
The traveller leaves at (3/5)c and returns at (3/5)c in order to meet up at the inertial-observer's 10-tickstick anniversary after separation. 
ClockEffect-AB-RRGP-rotatedGraphPaper-robphy

To help in "visualizing proper time", here is a spacetime diagram on rotated graph paper.
The key feature in the construction is that the area of the "light-clock diamonds" (marking off the ticks of a wristwatch) are equal in magnitude along different inertial worldlines.
The traveller leaves at (3/5)c and returns at (3/5)c in order to meet up 10-ticks after separation. ClockEffect-AB-RRGP-rotatedGraphPaper-robphy

To help in "visualizing proper time", here is a spacetime diagram on rotated graph paper.
The key feature in the construction is that the area of the "light-clock diamonds" (marking off the ticks of a wristwatch) are equal in magnitude along different inertial worldlines.
The traveller leaves at (3/5)c and returns at (3/5)c in order to meet up at the inertial-observer's 10-tick anniversary after separation. 
ClockEffect-AB-RRGP-rotatedGraphPaper-robphy

add references to "Relativity on Rotated Graph Paper"
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robphy
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For more information about these spacetime-diagrams on rotated graph paper,
check out my paper ("Relativity on Rotated Graph Paper", Am. J. Phys. 84, 344 (2016); http://dx.doi.org/10.1119/1.4943251 ; early draft: https://arxiv.org/abs/1111.7254 ).
See also my informal presentation at https://www.physicsforums.com/insights/relativity-rotated-graph-paper/ and my GeoGebra presentation at https://www.geogebra.org/m/HYD7hB9v#


For more information about these spacetime-diagrams on rotated graph paper,
check out my paper ("Relativity on Rotated Graph Paper", Am. J. Phys. 84, 344 (2016); http://dx.doi.org/10.1119/1.4943251 ; early draft: https://arxiv.org/abs/1111.7254 ).
See also my informal presentation at https://www.physicsforums.com/insights/relativity-rotated-graph-paper/ and my GeoGebra presentation at https://www.geogebra.org/m/HYD7hB9v#

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robphy
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If traveling inertially, the clock in the box doesn't know if it's moving.
That's the "Principle of Relativity"!


The following elaborates on Dale's answer.

Geometric analogies are useful.

  • On a geometrical plane, a straight-line path from point A to B
    (regardless of the direction from A to B)

    has a length which is computed by chaining together a sequence of short straight-line segments from A to B.
    (This means that the path from A to B doesn't have to be in any particular direction, like vertical or horizontal.)
  • In spacetime, an inertial path from event A to B
    (regardless of the inertial velocity from A to B as viewed in your frame) has an elapsed-wristwatch-time which is computed by chaining together a sequence of short inertial wristwatch-ticks from A to B.
    (This means that the inertial path from A to B doesn't have to be in any particular velocity, like "at rest".)

For piecewise paths...

  • Triangle inequality: Instead of going a along straight-line-path from A to C, you take (for simplicity) piecewise-straight-line-paths A to M, then M to B. From Euclidean geometry, it turns out that the straight-line-distances satisfy: $$dist(A,M)+dist(M,B) > dist(A,B).$$
    "The straight-line path has the shortest distance."
    So, the car from A to B will have less tire-wear than the car from A to M to B.

  • Clock Effect: Instead of going along an inertial-path from A to B, you take (for simplicity) piecewise-inertial-paths A to M, then M to B. From special relativity, it turns out that the inertial-path-elapsed-times satisfy: $$t(A,M)+t(M,B) < t(A,B). $$
    "The inertial path logs the longest elapsed-time."
    So, the inertial-observer from A to B will have aged more than the non-inertial observer from A to M to B.

  • Common-Sense Galilean-relativity: Instead of going along an inertial-path from A to B, you take (for simplicity) piecewise-inertial-paths A to M, then M to B. From Galilean relativity, it turns out that the inertial-path-elapsed-times satisfy: $$t(A,M)+t(M,B) = t(A,B).$$
    "The elapsed time logged from A to B is independent of the path from A to B."
    So, the inertial-observer from A to B will have aged as much as the non-inertial observer from A to M to B.


Admittedly, it's difficult to visualize the special relativity case because of the non-Euclidean geometry of Minkowski Spacetime. (It is underappreciated that the ordinary position-vs-time graph is also a non-Euclidean geometry... but we've learned to extract information from that diagram.)

To help in "visualizing proper time", here is a spacetime diagram on rotated graph paper.
The key feature in the construction is that the area of the "light-clock diamonds" (marking off the ticks of a wristwatch) are equal in magnitude along different inertial worldlines.
The traveller leaves at (3/5)c and returns at (3/5)c in order to meet up 10-ticks after separation. ClockEffect-AB-RRGP-rotatedGraphPaper-robphy


When they reunite, the non-inertial traveler (although piecewise-inertial) is younger than the [always] inertial observer.

Although this diagram is drawn from the stay-at-home frame, the result is independent of the frame of reference.
And there is no Lorentz transformation that will ever straighten out A-M-B to be an inertial path. A ball sitting on a frictionless surface on the traveller's ship will move when the ship necessarily-turns at M. (The analogous situation is true in Galilean relativity.)
(Just like in ordinary geometry... the lengths and angles in a triangle are the same if the figure is rotated. And no rotation will unkink A-M-B to be a straight-line.)
ClockEffect-AM-RRGP-rotatedGraphPaper-robphy