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4. Find the peak wavelength of the blackbody radiation emitted by (a) The Sun (2000 K)...
The surface of the sun has a temperature of approximately 5800 K. To good approximation we...
The surface of the sun has a temperature of approximately 5800 K. To good approximation we can treat it as a blackbody. (a) What is the peak-intensity wavelength λm? (b) What is the total radiated power per unit area? (c) Find the power per unit area radiated from the surface of the sun in the wavelength range 600.0 to 605.0 nm.
The Sun's surface is a blackbody with a surface temperature of 5800 K. a) at what...
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 intensity of blackbody radiation peaks at a wavelength of 608 nm. (a) What is the...
The intensity of blackbody radiation peaks at a wavelength of 608 nm. (a) What is the temperature (in K) of the radiation source? (Give your answer to at least 3 significant figures.) ______K (b) Determine the power radiated per unit area (in W/m2) of the radiation source at this temperature. _______ W/m2
(1) The intensity of blackbody radiation peaks at a wavelength of 668 nm. (a)What is the...
(1) The intensity of blackbody radiation peaks at a wavelength of 668 nm. (a)What is the temperature (in K) of the radiation source? (Give your answer to at least 3 significant figures.) (b)Determine the power radiated per unit area (in W/m2) of the radiation source at this temperature. (2) What is the binding energy in eV of electrons in ruthenium, if the longest-wavelength photon that can eject electrons is 264 nm?
Q1: The sun can be treated as a blackbody at an effective surface temperature of 10,400 R. The su...
Q1: The sun can be treated as a blackbody at an effective surface temperature of 10,400 R. The sun can be treated as a blackbody. (a) Determine the rate at which infrared radiation energy (0.76-100 um) is emitted by the sun, in Btu/hft. (b) Determine the fraction of the radiant energy emitted by the sun that falls in the visible range. (c) Determine the wavelength at which the emission of radiation from the sun peaks (d) Calculate and plot the...
2. The average person has 1.4 m2 of skin at a skin temperature of roughly 305...
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...
Construct plots that show the wavelength-dependent energy spectrum of a blackbody at a temperature of 5800...
Construct plots that show the wavelength-dependent energy spectrum of a blackbody at a temperature of 5800 K (approx. temperature of the Sun) using both the Planck distribution and the Raleigh-Jeans distribution. Confirm agreement between the two at long wavelength. a. What is the maximum emission wavelength at this temperature? b. What is the total power output (W/m^2) ? c. Using the Planck distribution, estimate what fraction of the Sun's total power output is emitted in visible wavelengths (400-750 nm)
Use the following information for the next three questions: The sun has a radius of 695,700...
Use the following information for the next three questions: The sun has a radius of 695,700 km and emits blackbody radiation at a temperature of 5778 K. Assuming that all of the sun's radiation is emitted at the peak wavelength, find the number of photons emitted by the sun per second. 9.7 x 1014 9.7 x 1024 9.7 x 1044
Estimate the peak wavelength for radiation from the following sources, assuming blackbody emission. (a) ice at...
Estimate the peak wavelength for radiation from the following sources, assuming blackbody emission. (a) ice at -4
The Wien displacement law states that the wavelength maximum in micrometers for blackbody radiation is A...
The Wien displacement law states that the wavelength maximum in micrometers for blackbody radiation is A T = 2.9 x 10 where Tis the temperature in kelvins. Calculate the wavelength maximum for a blackbody that has been heated to a 10000 K Wavelength = jum b. 6000 K Wavelength= um c. 2000 K Wavelength = um d. 1000 K Wavelength = um
Q1: The sun can be treated as a blackbody at an effective surface temperature of 10,400 R. The sun can be treated as a blackbody. (a) Determine the rate at which infrared radiation energy (0.76-100 um) is emitted by the sun, in Btu/hft. (b) Determine the fraction of the radiant energy emitted by the sun that falls in the visible range. (c) Determine the wavelength at which the emission of radiation from the sun peaks (d) Calculate and plot the...
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...
Construct plots that show the wavelength-dependent energy spectrum of a blackbody at a temperature of 5800 K (approx. temperature of the Sun) using both the Planck distribution and the Raleigh-Jeans distribution. Confirm agreement between the two at long wavelength. a. What is the maximum emission wavelength at this temperature? b. What is the total power output (W/m^2) ? c. Using the Planck distribution, estimate what fraction of the Sun's total power output is emitted in visible wavelengths (400-750 nm)
The Wien displacement law states that the wavelength maximum in micrometers for blackbody radiation is A T = 2.9 x 10 where Tis the temperature in kelvins. Calculate the wavelength maximum for a blackbody that has been heated to a 10000 K Wavelength = jum b. 6000 K Wavelength= um c. 2000 K Wavelength = um d. 1000 K Wavelength = um
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