Exitance is defined as the power per unit area that is emitted from the surface of an object. For a blackbody radiator, the exitance emitted is dependent upon its temperature. Calculate the exitance in W/cm2W/cm2 for a blackbody radiator at 74 K74 K and 323 K.323 K.
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W/cm2W/cm2
exitance at 323 K=
Exitance is defined as the power per unit area that is emitted from the surface of...
Exitance is defined as the power per unit area that is emitted from the surface of an object. For a blackbody radiator, the exitance emitted is dependent upon its temperature. Calculate the exitance in W / cm 2 for a blackbody radiator at 57 K and 319 K .
Chapter 26A Homem Christopher Cooper e-PHY 122 - Summer 19 - HAN Activities and Due Dates Chapter 26A Homework gnment Score: 1145/1500 Resources Hint Check Answe stion 8 of 15 > Exitance is defined as the power per unit area that is emitted from the surface of an object. For a blackbody radiator, the exitance emitted is dependent upon its temperature. Calculate the exitance in W/cm' for a blackbody radiator at 69 K and 328 K. exitance at 69 K...
The total power emitted by the sun is 4x1026 W. Calculate the Solar Constant, defined as the power per unit area that reaches the earth outside the atmosphere. The distance from sun to earth is 1.49x1011 m.
Radiation of Energy The rate of heat transfer by emitted radiation is determined by the Stefan-Boltzmann law of radiation: = aeAT4 where o 5.67x10-8 J/s - m2 K is the Stefan-Boltzmann constant, A is the surface area of the object, and T is its absolute temperature in kelvin. The symbol e stands for the emissivity of the object, which is a measure of how well it radiates An ideal jet-black (or black body) radiator has e 1,whereas a perfect reflector has...
2. The average person has 1.4 m2 of skin at a skin temperature of roughly 305 K (90°F) Consider the average person to be an ideal radiator standing in a room at a temperature of 293 K (68°F) (a) Calculate the power (energy per uni i) radiated by the average person in the form of blackbody radiation; express your answer in erg s-1. What is the person's "wattage"? (1 W = 107 erg s-1) Compare this to a typical incandescent...
12.I7 An enclosure has an inside area of 50 m, and its inside surface is black and is maintained at a con- stant temperature. A small opening in the enclosure has an area of 0.0 m2. The radiant power emitted from this opening is 52 W. What is the temperature of the interior enclosure w If the interior surface is maintained at this temperature, but is now polished so that its emissivity is 0.15, what will be the value...
The energy radiated per unit surface area (across all wavelengths) for a black body with temperature 2200. Use 5.67 x 10-8 for the Stefan-Boltzmann constant. The Stefan-Boltzmann Law describes the power radiated from a black body in terms of its temperature. Specifically, the total energy radiated per unit surface area of a black body across all wavelengths per unit time is proportional to the fourth power of the black body's thermodynamic temperature
Calculate the average power that the surface of Earth facing the Sun receives from the Sun. Assuming that the Earth is a blackbody and radiates the same amount of power that it absorbs from the Sun, calculate the average surface temperature of the Earth. Does your answer make sense compared to your experience? The Sun’s surface temperature is 5800 K, its radius is 6.96x108 m, the distance between Earth and the Sun is 1.5x1011 m, and the radius of the...
The Sun's surface is a blackbody with a surface temperature of 5800 K. a) at what wavelength does the sun emit most strongly? b) what is the total radiated power per unit surface area? c) what is the total radiated power over the entire surface?
The rate of heat transfer by emitted radiation is determined by the Stefan-Boltzmann law of radiation = ceAT4 t where a 5.67x108 J/(s m2. K4) is the Stefan-Boltzmann constant, A is the surface area of the object, and T is its absolute temperature in kelvin. The symbol e stands for the emissivity of the object, which is a measure of how well it radiates. An ideal jet-black (or black body) radiator has e 1, whereas a perfect reflector has e...