Step 1:
We start by using the formula for length contraction in special relativity, which is given by:
\[L = L_0 \sqrt{1 - \frac{v^2}{c^2}}\]
where \(L\) is the contracted length, \(L_0\) is the rest length, \(v\) is the relative velocity, and \(c\) is the speed of
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