Since the sun is almost directly overhead, then we can say that we have two right triangles that are similar.
So, we can formulate the following equation:
[tex]\begin{gathered} \frac{h1}{b1}=\frac{h2}{b2}\text{ (h1: 2 ft, b1: 11 in=0.92 ft, h2: height of the top of the pole, b2: shadow of the pole )} \\ \frac{2\text{ ft}}{0.92\text{ ft}}=\frac{h2}{7\text{ ft}}\text{ (Replacing)} \\ \frac{2\text{ ft}}{0.92\text{ ft}}\cdot7\text{ ft= h2 (Multiplying by 7 ft on both sides of the equation)} \\ 15.22\text{ ft = h2 (Dividing and multiplying )} \end{gathered}[/tex]
The height is 15.21 ft.
Converting the answer to inches, we have:
[tex]15.22ft\cdot\frac{12\text{ in}}{1\text{ ft}}=182.6\text{ in}[/tex]
The answer is 183 inches (Rounding to the nearest inch)