Question

Consider a blackbody surface that emits 54.880% of its emissive power at wavelengths that are shorter than 3.3008 microns. What is the temperature of the surface in Cº?

Consider a blackbody surface that emits 54.880% of its emissive power at wavelengths that are shorter than 3.3008 microns. What is the temperature of the surface in Cº?

0 0
Add a comment Improve this question Transcribed image text
Answer #1

youn uen = 0.54830 A= 3.3008 丸feetal 1.aual 43 954m, K 9-3008 m T- , ㅜ드 1331475 K As E d

Add a comment
Know the answer?
Add Answer to:
Consider a blackbody surface that emits 54.880% of its emissive power at wavelengths that are shorter than 3.3008 microns. What is the temperature of the surface in Cº?
Your Answer:

Post as a guest

Your Name:

What's your source?

Earn Coins

Coins can be redeemed for fabulous gifts.

Not the answer you're looking for? Ask your own homework help question. Our experts will answer your question WITHIN MINUTES for Free.
Similar Homework Help Questions
  • The wavelength at which the blackbody emissive power reaches its maximum value at a temperature of...

    The wavelength at which the blackbody emissive power reaches its maximum value at a temperature of 300 K is 9.7 um 38.0 um 73.1 um 15.5 um 5.1 um

  • (a) Schematically draw the spectral emissive power of two blackbodies with the temperature of 2400 K...

    (a) Schematically draw the spectral emissive power of two blackbodies with the temperature of 2400 K and 300 K (ie. EBA versus λ). What are the wavelengths at the maximum spectral emissive power? (5 pts) (b) A thin-walled plate separates the interior of a large furnace from surroundings at 300 K. The plate is fabricated from a ceramic material for which diffuse surface behavior may be assumed and the exterior surface is air-cooled. With the furnace operating at 2400 K...

  • 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...

  • 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?

  • What was the temperature anomaly in Buffalo, NY on August 27 , 2019? Give your answer...

    What was the temperature anomaly in Buffalo, NY on August 27 , 2019? Give your answer in °C. Answers within ±3°C of the correct answer are marked correct. The long-term average temperature for August in Buffalo is 20 °C. Using this information and your answer from Q8, what was the temperature in Buffalo on August 27, 2019? Give your answer in °C. Hotter objects emit _________ than cooler objects a. more energy at redder wavelengths b. more energy at bluer...

  • A small object with an opaque, diffuse surface at a temperature of 500 K is suspended...

    A small object with an opaque, diffuse surface at a temperature of 500 K is suspended in a large furnace with walls at 2000 K. Assume that the walls of the furnace provide a diffuse irradiation to the object at a blackbody temperature equal to the furnace wall temperature. The object’s surface has a spectral hemispherical emissivity and absorptivity as given below. (a) Determine the total emissivity and total absorptivity of the object’s surface. Partial Ans: ?=0.021 (b) Evaluate the...

  • The energy radiated per unit surface area (across all wavelengths) for a black body with temperature...

    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

  • Problem 2: A small surface A1, with area 7 cm2, emits radiation as a blackbody at 800K. Part of its radiation hits anot...

    Problem 2: A small surface A1, with area 7 cm2, emits radiation as a blackbody at 800K. Part of its radiation hits another small surface A2, with area 7 cm2, which is oriented as shown in the figure below. (a) Determine the solid angle of A2 as viewed from Aı. (b) Determine the radiation heat transfer rate (in W) from A1 to A2. Hint: you can assume the surfaces are small relative to their separation distance Problem2 02-60A2 r-80 cm...

  • 1. The "surface" of the Sun is not sharp boundaries like the surface of the Earth....

    1. The "surface" of the Sun is not sharp boundaries like the surface of the Earth. Most of the radiation that the Sun emits is in thermal equilibrium with the hot gases that make up the Sun's outer layers. Without too much error, we can treat sunlight as blackbody radiation. The total power radiated by the Sun is 3.87×1026W. Given the radius of the Sun is 6.96×108m, what is the surface temperature of the Sun? Suppose the temperature of the...

  • Consider a spherical blackbody of temperature T=230 oC and radius R=0.20m that radiates energy to an...

    Consider a spherical blackbody of temperature T=230 oC and radius R=0.20m that radiates energy to an environment of very low temperature. Suppose you surround the sphere with a black, thin, spherical shell of radius 6R. What is the temperature of the shell in Celsius when it reaches a steady state? Remember the inner surface of the large sphere is always absorbing energy from the black body and the outer surface is loosing energy to the very low temperature surroundings.   oC

ADVERTISEMENT
Free Homework Help App
Download From Google Play
Scan Your Homework
to Get Instant Free Answers
Need Online Homework Help?
Ask a Question
Get Answers For Free
Most questions answered within 3 hours.
ADVERTISEMENT
ADVERTISEMENT
ADVERTISEMENT