Step 1: Understanding the Concept:
In Bohr's model, the electron's orbit holds a whole number of de Broglie wavelengths, so \(2\pi r_n = n\lambda_n\).
Step 2: Key Formula or Approach:
\[ \lambda_n = \frac{2\pi r_n}{n},\qquad r_n\propto n^2 \]
Step 3: Detailed Explanation:
\[ \lambda_n\propto\frac{n^2}{n} = n \]
So the wavelength is proportional to the orbit number:
\[ \frac{\lambda_3}{\lambda_1} = \frac31 \Rightarrow \lambda_3 = 3\lambda_1 \]
Alternative check: the speed in orbit \(n\) is \(v_n\propto\dfrac1n\), so the momentum \(mv\) falls as \(1/n\), and \(\lambda = \dfrac{h}{mv}\) rises as \(n\). The result is the same.
Final Answer:
\(\lambda_3 = 3\lambda_1\), option (D).
\[ \boxed{3\lambda_1 \text{ (D)}} \]