he energy flux F from a blackbody at temperature T is proportional to the fourth power of its absolute temperature. This relationship is known as the Stefan-Boltzmann law and can be written in the form of an equation as F = T4 where F stands for the energy flux (in units of watts per square meter: W/m2), T is given in Kelvins: K, and (Greek letter sigma) is a constant number, = 5.67 10-8 W /(m2 K4). Find the temperature T in K of a blackbody if the energy flux F from this blackbody is F = 170 W/m2. Type only the numerical part of your answer using scientific E-notation with 3 significant figures