You can start with the Principle of Relativity. You can easily find the excellent account written by Galileo of being in the hold of a ship. Once you learn that there is no difference between uniform motion and rest, then move on to the second postulate of Einstein's relativity. It's an assertion that tells us no matter how fast we travel chasing a light beam, the beam will recede from us at the same speed as it did when we were not chasing it. There's a quip about understanding this idea, and it goes like this. If you think you understand it when you first encounter it, then you don't.
Let's refer to them as A, B, and C. B is in the middle. The speed of A with respect to B is 0.8
c. Likewise, the speed of C with respect to B is 0.8
c.
View attachment 91314
Paradoxically, B will see the separation distance between A and C increase at a rate of 1.6
c.
But A will see C recede at a speed of about 0.98
c. Likewise, C will see A recede at at a speed of about 0.98
c.
The easiest way to do the math is to introduce the speed parameter ##\theta## defined by the equation
$$\beta=\tanh \theta.$$
In this example ##\beta=0.8##. Use the above relation to find that ##\theta \approx 1.0986##. Instead of adding 0.8 + 0.8 to find the relative speed of A with respect to C, we add 1.0986 + 1.0986 to get 2.1972. Then again use the above relation to find ##\beta##.
$$\beta=\tanh (2.197) \approx 0.98.$$
So in Galilean relativity we add the speeds ##\beta## but in Einsteinian relativity we add the speed parameters ##\theta##.
This is an example of the use of hyperbolic spacetime geometry.