At what temperature must a body be heated to generate black-body spectrum with a maximum wavelength of 160nm.
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At what temperature must a body be heated to generate black-body spectrum with a maximum wavelength of 160nm.
2. The maximum wavelength of an ideal black body cavity radiation absorption is 6000 A. a. If the emission of thermal radiation from the cavity becomes 3 times, then what is the maximum wavelength and temperature? b. If the emission of thermal radiation from the cavity becomes times, then what is the maximum wavelength and temperature?
What is the temperature If the peak of a blackbody spectrum is at 17.0 m? What is the wavelength at the peak of a blackbody spectrum if the body is at a temperature of 1700 K? About 0.1ev is required to break a "hydrogen bond" in a protein molecule. Calculate the minimum frequency and maximum wavelength of a photon that can be accomplish this minimum frequency
A star has the maximum emission at a wavelength lmax=300 nm. Calculate the surface temperature of the star, assuming that the star behaves like an ideal black body.
A blackbody radiator is at body temperature (38 C). What is the wavelength at which the maximum power per unit wavelength is emitted.
A black body has an effective surface temperature of 450°C. Determine: (a) The total radiation energy (W/m2) that can be emitted by the black body (b) Determine total radiation energy (W/m%) that can be emitted by the black body within the 5-50 um wavelength region (c) The spectral blackbody emissive power of the black body at a wavelength of 10 um. 12
8. A black body has an effective surface temperature of 450°C. Determine: (a) The total radiation energy (W/m²) that can be emitted by the black body (b) Determine total radiation energy (W/m²) that can be emitted by the black body within the 5-50 um wavelength region (c) The spectral blackbody emissive power of the black body at a wavelength of 10 um.
8. Compute the ratio of the increase of intensity of black-body radiation at a wavelength of 641 nm for an increase of temperature from 1200 to 1500 K
7. What is the relation between temperature and intensity of black body radiation? 8. What is the relation between the temperature of a black body and the color of its radiation? 9. What is the closest thing to a black body in our everyday life? 10. What is the importance of Planck's radiation law for modern Physics?
A star can be approximated to a black body mostly constituted of gas with a surface temperature T. From the black body density of oscillators we can demonstrate that the power emitted in the forward direction by the star of surface area A per unit wavelength is: A exp( )-1 (Eg.1) Maximum emission Using Equation I , give an approximation of the power Permitted at short wavelengths (λ<<1). c.
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)