We want to express the coordinates
and
of an inertial frame
in terms of the coordinates
and
of another inertial frame
We will assume that the two frames meet the following conditions:
- their spacetime coordinate origins coincide (
mark the same spacetime location as
),
- their space axes are parallel, and
moves with a constant velocity
relative to 
What we know at this point is that whatever moves with a constant velocity in
will do so in
It follows that the transformation
maps straight lines in
onto straight lines in
Coordinate lines of
in particular, will be mapped onto straight lines in
This tells us that the dashed coordinates are linear combinations of the undashed ones,

We also know that the transformation from
to
can only depend on
so
and
are functions of
Our task is to find these functions. The real-valued functions
and
actually can depend only on
so
and
A vector function depending only on
must be parallel (or antiparallel) to
and its magnitude must be a function of
We can therefore write
and
(It will become clear in a moment why the factor
is included in the definition of
) So,

Let's set
equal to
This implies that
As we are looking at the trajectory of an object at rest in
must be constant. Hence,

Let's write down the inverse transformation. Since
moves with velocity
relative to
it is

To make life easier for us, we now chose the space axes so that
Then the above two (mutually inverse) transformations simplify to


Plugging the first transformation into the second, we obtain


-



The first of these equations tells us that
and 
The second tells us that
and 
Combining
with
(and taking into account that
), we obtain
Using
to eliminate
we obtain
and
Since the first of the last two equations implies that
we gather from the second that
tells us that
must, in fact, be equal to 1, since we have assumed that the space axes of the two frames a parallel (rather than antiparallel).
With
and
yields
Upon solving
for
we are left with expressions for
and
depending solely on
:

Quite an improvement!
To find the remaining function
we consider a third inertial frame
which moves with velocity
relative to
Combining the transformation from
to

with the transformation from
to

we obtain the transformation from
to
:
![{\displaystyle t''=a(v)\left[a(w)\,t+{1-a^{2}(w) \over a(w)\,w}x\right]+{1-a^{2}(v) \over a(v)\,v}{\Bigl [}a(w)\,x-a(w)\,wt{\Bigr ]}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/aac5ef850e58cf4313f158ff823495cfda63278d)
-
![{\displaystyle =\underbrace {\left[a(v)\,a(w)-{1-a^{2}(v) \over a(v)\,v}a(w)\,w\right]} _{\textstyle \star }t+{\Bigl [}\dots {\Bigr ]}\,x,}](https://wikimedia.org/api/rest_v1/media/math/render/svg/f598d3a652be5ce24fbf91ac01439a8d4772177d)
![{\displaystyle x''=a(v){\Bigl [}a(w)\,x-a(w)\,wt{\Bigr ]}-a(v)\,v\left[a(w)\,t+{1-a^{2}(w) \over a(w)\,w}x\right]}](https://wikimedia.org/api/rest_v1/media/math/render/svg/7d163387fa694115abbe60fb231559ed50fe5046)
-
![{\displaystyle =\underbrace {\left[a(v)\,a(w)-a(v)\,v{1-a^{2}(w) \over a(w)\,w}\right]} _{\textstyle \star \,\star }x-{\Bigl [}\dots {\Bigr ]}\,t.}](https://wikimedia.org/api/rest_v1/media/math/render/svg/ae3bd80d12d1822ff47c0e945207167ce442828d)
The direct transformation from
to
must have the same form as the transformations from
to
and from
to
, namely

where
is the speed of
relative to
Comparison of the coefficients marked with stars yields two expressions for
which of course must be equal:

It follows that
and this tells us that

is a universal constant. Solving the first equality for
we obtain

This allows us to cast the transformation

into the form

Trumpets, please! We have managed to reduce five unknown functions to a single constant.