Question

Problems 6.14 (a) At what wavelength does the continuous spectrum from sunspots peak? (b) What is...

Problems 6.14

(a) At what wavelength does the continuous spectrum from sunspots peak?

(b) What is the ratio of intensities at 550 nm in a sunspot and in the normal photosphere?

(c) What is the ratio of energy per second per surface area

Homework Answers

Answer #1

a) using the wien's displacement law,

Wavelength max = b/T ,where b= 2900 \mum.K & T= temperature in K.

Considering,the surface temperature of sunspot to be 4000K,

Wavelength max= 2900 *10^(-6)/4000 = 7.22 × 10^(-7) m.

b) to know the ratio of intensities at 550nm ,the energy distribution in sunspot spectrum should be known.

c)ratio of energies= (ratio of temperatures)^4

From Stephan Boltzmann law,

Ratio of energies = (temperature of sunspot/temperature of sun surface)^4

Ratio of energies =(4000/5800)^4 = 0.22621

Know the answer?
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
Similar Questions
Suppose a star with radius 8.50 × 108 m has a peak wavelength of 685 nm...
Suppose a star with radius 8.50 × 108 m has a peak wavelength of 685 nm in the spectrum of its emitted radiation. Assume the star is a perfect blackbody. (A) What is the energy of a photon with this wavelength? (B) What is the surface temperature of the star? (C) At what rate is energy emitted from the star in the form of radiation?
1. What is the peak wavelength emitted by a star with a surface temperature of 7070...
1. What is the peak wavelength emitted by a star with a surface temperature of 7070 K? Give your answer in nm (1 nm = 10-9 m), but enter only the numerical part in the box. 2. By how much would a star's temperature need to increase in order for its peak wavelength to decrease from 460 to 360 nm? Your answer will be the change in temperature. Give your answer in K, but enter only the numerical part in...
The wavelength of peak emission from any star is related to the temperature of its photosphere...
The wavelength of peak emission from any star is related to the temperature of its photosphere (i.e., the emitting surface) by Wien’s Law, given by λ = 2,900/T, where λ is the wavelength in micrometers (1 µm = 10-6 m), and T is the temperature of the star in Kelvin (see textbook’s figure 3.27 for help). Answer the following questions using the above equation. 2.1. The most massive star ever observed is a Wolf-Rayet type-star, named R136a1. It is so...
Assuming blackbody emission, find the wavelength of peak radiation from the following objects: a) surface of...
Assuming blackbody emission, find the wavelength of peak radiation from the following objects: a) surface of the sun at 5778 K, b) boiling water at 100 degrees C, c) helium at 4 K d) the universe at T=2.725 K. In what region of the electromagnetic spectrum is each?
a) at approximately what location is the carbonyl peak of cyclohexanone on the IR spectrum? b)...
a) at approximately what location is the carbonyl peak of cyclohexanone on the IR spectrum? b) at approximately what location is the OH peak of cyclohexanol on the IR spectrum? c) is it jagged or rounded? d) what two classes of compounds can primary alcohols be oxidized? e) what determines which product results from such oxidation?
The hydrogen atomic emission spectrum includes a UV line with a wavelength of 92.323 nm. Photons...
The hydrogen atomic emission spectrum includes a UV line with a wavelength of 92.323 nm. Photons of this wavelength are emitted when the electron transitions to nf = 1 as the final energy state. Show all steps and round answers to correct sig figs. a) Is this line associated with a transition between different excited states or between an excited state and the ground state? b) What is the energy of the emitted photon with wavelength 92.323 nm? c) What...
d) Use the Spectrum Simulation to investigate changes in the amount of light at visible wavelengths...
d) Use the Spectrum Simulation to investigate changes in the amount of light at visible wavelengths due to this change in temperature from 2500 C to 2000 C. i) What is the approximate ratio between the powers emitted at 500 nm at 2000 degrees C to that at 2500 degrees C, that is, the power emitted at 500 nm at 2000 degrees C divided by the amount of power at 500 nm at degrees 2500 C? ii) In question 1b,...
Betelgeuse Written Homework The spherical star Betelgeuse has the following properties: peak wavelength = 807 nm...
Betelgeuse Written Homework The spherical star Betelgeuse has the following properties: peak wavelength = 807 nm radius = 6.3E11 m mass = 2.31E31 kg distance to Earth = 6.85E18 m emissivity = 1 Determine the following based on the above information and relevant equations: a) Temperature of the light-emitting surface of Betelgeuse, assumed constant (as an aside, note that there isn't really a single temperature of a star). b) Power of Betelgeuse. c) Intensity of light from Betelgeuse reaching Earth...
A star has a surface temperature of 4500 K. a. Calculate the peak wavelength of its...
A star has a surface temperature of 4500 K. a. Calculate the peak wavelength of its brightness vs. wavelength curve. [1.5 points] b. What color does this wavelength correspond to? (Note: See p. 5-7 of the textbook for a list of colors corresponding to different wavelength ranges. If the wavelength is in the infrared or ultraviolet range, state “IR” or “UV” as the color.) [0.5 points] c. Now imagine that the star is moving away from us at 0.15c, where...
The star Rigel acts like a Blackbody. Its surface temperature is 10,000k A) Calculate the total...
The star Rigel acts like a Blackbody. Its surface temperature is 10,000k A) Calculate the total power per unit area emitted by Rigel B) Calculate the wavelength of peak intensity for Rigel's blackbody spectrum. C) Calculate the energy of a photon of wavelength given in B) above.