(a) Both will emit equal amount of radiation per unit time in the beginning.
(b) Both will absorb equal amount of radiation from the surrounding in the beginning.
Let the temperature of the surroundings be .
From the Stefan-Boltzmann law, the energy of thermal radiation emitted per unit time by a blackbody of surface area A is given by
Here, is Stephen's constant.
Also, the energy absorbed per unit time by the body is given by
As the two spheres have equal radii and temperatures, their rate of absorption and emission will be equal in the beginning.