- Heat Transfer - Section 1
- Heat Transfer - Section 2
- Heat Transfer - Section 3
- Heat Transfer - Section 4
- Heat Transfer - Section 5
- Heat Transfer - Section 6
- Heat Transfer - Section 7
- Heat Transfer - Section 8
- Heat Transfer - Section 9
- Heat Transfer - Section 10
- Heat Transfer - Section 11


Heat Transfer - Engineering
Q1: The thermal radiation emitted by a body is proportional to Tn, where T is its absolute temperature. The value of 'n' is exactly 4 forA black painted bodies only
B all bodies
C polished bodies only
D a black body
ANS:B - all bodies The value of 'n' being exactly 4 for "all bodies" is not accurate. The correct statement is that for all idealized bodies, specifically black bodies, the value of 'n' is exactly 4. A black body is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. It also emits radiation at the maximum possible intensity for any given temperature, according to Planck's law. The Stefan-Boltzmann law states that the total rate of radiation emitted per unit surface area of a black body is directly proportional to the fourth power of the absolute temperature (T) of the body. Mathematically, this is expressed as: 4Q=σT4 Where:
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