Step 1: Understanding the Stefan-Boltzmann law.
The emissive power \( E \) of a body is given by the Stefan-Boltzmann law:
\[
E = \sigma \epsilon T^4
\]
where \( \sigma \) is the Stefan-Boltzmann constant, \( \epsilon \) is the emissivity, and \( T \) is the temperature of the body.
Step 2: Relating the emissive power and temperature.
Given that the emissive power is the same for both spheres, we can write:
\[
\sigma \epsilon_1 T_1^4 = \sigma \epsilon_2 T_2^4
\]
Since the emissivity ratio is 1:4, we substitute \( \epsilon_1 = 1 \) and \( \epsilon_2 = 4 \) into the equation:
\[
T_1^4 = 4 T_2^4
\]
Step 3: Solving for the temperature ratio.
Taking the fourth root of both sides:
\[
T_1 = \sqrt{4} T_2 = 2 T_2
\]
Thus, the ratio of \( T_1 \) to \( T_2 \) is \( \sqrt{2} : 1 \), which corresponds to option (A).