Answer:
Step-by-step explanation:
For black body radiation, we shall apply Stefan's law, which is defined as follows
E = σ Τ⁴
The value of σ which is also known as stefan's constant is .567 x 10⁻⁷ m⁻²k⁻⁴
and T is absolute temperature. E is heat energy emitted from the surface of a black body per unit area per second.
At temperature 66k
E = .567 X 10⁻⁷ X (66)⁴
= 1.897 X 10⁷ X .567 X 10⁻⁷
= 1.076 J /s m²
1.076 x 10⁻⁴ J s⁻¹ cm⁻²
exitance = 1.076 x 10⁻⁴ Wcm⁻²
Similarly we can calculate exitance of black body at 317 K as follows
E = .567 X 10⁻⁷ X (317)⁴
= .567 X 10³ Wm⁻²
exitance = .567 x 10⁻¹ W cm⁻⁴