Correct answer: 10⁻⁶ rad
The angular resolution is given by the formula θ = 1.22 * λ / D, where λ is the wavelength and D is the diameter of the telescope. Substituting λ = 5000 Å = 5 × 10⁻⁷ m and D = 0.1 m, we get θ ≈ 1.22 × (5 × 10⁻⁷) / 0.1 ≈ 6.1 × 10⁻⁶ rad, which is closest to 10⁻⁶ rad.