As I understand it, an ideal blackbody absorbs (and subsequently starts emitting) all incoming radiation. In typical setups like determining a planet's temperature given its albedo and distance from a star, we use the thermal equilibrium condition $P_{in} = P_{out}$ for the planet and use Stefan-Boltzmann's Law to obtain the planet's temperature (using approximations like emissivity, albedo, and so on).
Now, suppose we have an ideal spherical blackbody (A) inside a larger ideal blackbody in the shape of a spherical shell (B). This entire setup is in deep space. Say A has some source of power like fusion going on inside similar to a star. Here, the power emitted by A, $P_A$, is equal to the power supplied by the fusion reaction. Also, suppose that initially $P_A >> P_B$ (we can neglect any radiation by B initially; suppose no fusion is going on inside it). Now, as the outgoing $P_A$ is incident on B, after a while (when thermal equilibrium is reached), B starts emitting radiation with power $P_A$ (here, B emits $\frac{P_A}{2}$ outwards into deep space, and $\frac{P_A}{2}$ is emitted towards A). So, this $\frac{P_A}{2}$ is incident on A, which after a while starts emitting at $P_A + \frac{P_A}{2} = \frac{3}{2}P_A$. Then, this $\frac{3}{2}P_A$ will be incident on B, causing its emitting power to eventually raise to $\frac{3}{2}P_A$. From here, half of the power, i.e. $\frac{3}{4}P_A$ will again heat up A further. This in turn will heat up B, which will again heat up A. And so on and so forth.
Apparently, therefore, I am unable to see how the two interacting blackbodies will ever reach equilibrium. This is quite puzzling, and I think I might have some loopholes in the fundamental understanding of blackbodies in the first place. Any help is appreciated.