Interpretation of the Experiment
In
order to understand what the experiment means, we must write down the equation
of the curve defined by projecting the wavefront curve at
to the (standard) coordinates of the
plane of
. I do this by introducing certain coordinates for the
plane of
. We saw this in a Euclidean context in (3.2) of Planes Intersecting Cones.
The "speed" of
(as measured by
) is defined to be
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I assume for this experiment
that
otherwise, there is nothing to do.
We saw that the wavefront curve was an ellipse in the (stationary)
frame of
by using the basis
in
coordinates, given by
![]()
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where these vectors satisfy the hyperbolic orthogonality relations:
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We
see that there are orthogonal unit vectors U and V in the
plane of
so that the projected ellipse is given by the parametric equation
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(7.2) |
From this it follows that the projected curve
is an ellipse with major axis on the line generated by
. This is illustrated below:

The
interpretation of this is the following. The projected ellipse is the projection
to the
plane of the
observer of his measured spatial positions of the wavefront at the
observer's time
. It is not a circle because this wavefront does not consist of simultaneous
events for
(I assumed that
).
The major axis of this ellipse contains, between the focus
at the origin and the second focus, the line of spatial positions of the world-line
of
between his time
.
In particular, he moves from the origin (first focus) to the center in 1 unit
of his time, which is
units of the
observer's time. His projection must therefore move to the second focus at his
time
.
The
rays of light, emitted at various angles from the emission event, project to
segments connecting the first to the second focus via a point on the boundary
of the projected ellipse. The questions, of course, are: Why should the sum
of the lengths be constant? And what does this constant represent? And the answer
will now be fairly easy to see.
Consider
a ray of light that bounces from the emission to the reception event. Describe
its itinerary in the reference frame of observer
.
It starts from the origin event
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and arrives at the mirror at event,
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Next,
it reflects to the reception event:
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In the first leg of its itinerary, it lies in the light cone, so
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Since the square roots of both sides are equal, we conclude
that the spatial
projection of that path has length the absolute value:
. This is simply
since
.
In the second leg of its itinerary, it also lies in a light cone, so
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I conclude for the same reason that the spatial projection
of that path has length
.
Therefore, the sum of the spatial lengths is
. This is equal to the time that observer
measures from the emission event to the reception event. That
is, of course, the time coordinate in the frame of
of the event
. But from the definition of
in the previous section
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we see that this is:
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And
this, of course, is the length of the major axis of the projected ellipse. That
is a physical interpretation of why the sum of the lengths of the paths from
a point on the ellipse to its foci is constant. It is the time
measures between the emission and reception event, which is the same for all
rays of light.
Next,
I consider the focus-directrix property of the ellipse. I showed in Planes
Intersecting Cones that the intersection of the plane of simultaneity for
:
with the plane of simultaneity for
:
,
is a line that I call
.
![]()
I
represented the tangent plane, the plane
of simultaneity for
:
as the graph of a function of x and y:
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In
the present context, the function
has the following interpretation. With each point
there is a unique point on the plane of simultaneity for
:
that projects to it.
is the time coordinate that standard observer
ascribes to it. The line
is the set of events with
and
.
The calculation above shows
that the value of the eccentricity
is the speed of
as measured by ![]()
= ![]()
and it gives us the focus-directrix property of the projected ellipse.
Now,
we might ask how general this construction is. It is clear that for any particular
direction of motion of
with respect to
, we will obtain among the projected
ellipses one representative of the similarity class of ellipses for each speed
.
And every similarity class will be represented, simply by choosing the representative
with semi-minor axis of length 1, and semi-major axis of length
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Therefore this physical argument is completely general.
What happens if
is stationary with respect to
? In that case, this construction
breaks down when we attempt to build the
observer's orthonormal basis. But in that case, there is no need to build such
a basis. The foci collapse to the center, the ellipse is a circle, and everything
happens as it does in the frame of
.