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# Applying Relativity to Vector Math | ||
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Now that we've come to grips with the fundamental concepts and intuitions of | ||
relativity, we can start applying these concepts to vector math. | ||
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```admonish note | ||
So far we've seen how the speed of light postulate leads to time dilation and | ||
length contraction, but we've only scratched the surface of the implications of | ||
special relativity. | ||
For example, _momentum_ and _energy_. Momentum, $p = mv$, and kinetic energy, $K | ||
= \frac{1}{2}mv^2$, are both conserved quantities in Newtonian mechanics. Pay | ||
close attention and you'll see that both of these quantities depend on the | ||
_velocity_ of the object---relativity will affect these quantities too! | ||
This rabbit hole goes _deep_, eventually leading to the classic $E=mc^2$ | ||
equation and more, but we'll only cover the fundamentals and specific | ||
applications of relativity that relate to timekeeping and navigation in deep | ||
space. | ||
``` |
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