Suppose a star with radius 8.44 x 10^8 m has a peak wavelength of 677 nm in the spectrum of its emitted radiation.
(a) Find the energy of a photon with this wavelength.
J/photon
(b) What is the surface temperature of the star?
K
(c) At what rate is energy emitted from the star in the form of radiation? Assume the star is a blackbody (e = 1).
W
(d) Using the answer to part (a), estimate the rate at which photons leave the surface of the star.
photons/s
(A) energy of photon = hc/
= 6.626*10^-34*3*10^8 / 677*10^-9
= 2.93*10^-19 J/photon
(b) using wein's displacement law we have
max
*T = 2898*10^-6 m
677*10^-9*T = 2898*10^-6
T= 4280.65 K
(C) rate at which energy is radiated = 
AT^4
= 
4pi*r^2T^4
= 5.67*10^-8*4pi*(8.44*10^8)^2 * ( 4280.65)^4
= 1.7*10^26 W
(D) no. of photons per second = 1.7*10^26 / 2.93*10^-19
= 5.8*10^44
Suppose a star with radius 8.44 x 10^8 m has a peak wavelength of 677 nm...
below. 16.) Calculate the wavelength of the He-Ne laser, as shown in the figure Collision Helium p Neon 1.96 eV E3 E2 20.61 eV 20.66 eV 18.70 ev Eo 0 17.) Suppose a star with radius 8.50 x 108 m has a peak wavelength of 685 nm in the spectrum of its emitted radiation. (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...
The intensity of blackbody radiation peaks at a wavelength of 633 nm. a)Determine the energy associated with each photon. (Answer= 0.0912 eV) b) Assuming the sphere's power output is associated with the peak wavelength, determine the temperature of the sphere at which this wavelength is emitted.
in a mission, it has accelerated photons that bump with its solar tail. peak wavelength in the sun's spectrum is 501 nm. what is the momentum (in kg m/s) of a photon with a wavelength peak of 501 nm? also using the peak wavelength, what is the surface temperature of the sun?
(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?
A star has a surface temperature of 4,211 K. What is peak wavelength in nm of the light it emits? Give the answer to two significant figures. Use scientific notation, with one digit to the left and one digit to the right of the decimal point.
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
A photon has energy of 3.26 x 10^-19 J. a.) Compute the wavelength (in nm) of the radiation as the wave travels through a vacuum. b.) Within what region of the electromagnetic spectrum is this located?
Please Help. Blackbody Radiation.
Star A is a blackbody that has a power vs. wavelength curve as intensity shown in the two diagrams to the right. Now consider Star B, which is the same size as Star- A but is hotter. On the top graph, sketch what it's blackbody curve will look like in reference to Star A. Now consider Star C, which is at the same temperatur e as Star- A but has a larger radius. On the bottom...
One type of sunburn occurs on exposure to UV light of wavelength in the vicinity of 300 nm . Part A What is the energy of a photon of this wavelength? E = 6.03•1019 J SubmitMy AnswersGive Up Incorrect; Try Again; 4 attempts remaining Part B What is the energy of a mole of these photons? E = J SubmitMy AnswersGive Up Part C How many photons are in a 1.10 mJ burst of this radiation? N = photons SubmitMy...
37. Suppose a very young star has a peak wavelength of 0.97E-6m. In what region of the spectrum is this peak wavelength? a. What is its temperature? b.