EBK THE COSMIC PERSPECTIVE
EBK THE COSMIC PERSPECTIVE
9th Edition
ISBN: 9780135161760
Author: Voit
Publisher: VST
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Chapter 5, Problem 60EAP

(a)

To determine

To Calculate:The average power radiated by each square meter of sun’s surface.

(b)

To determine

To Calculate: The average surface temperature of the sun using answer from part a, and Stefan Boltzmann law,

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Use Wien's Law to calculate the peak wavelength of light coming from the Sun. Assume T=5800 K for the surface temperature of the Sun. Wein's displacement law says that the blackbody temperature and peak wavelength multiplied together give a constant of 0.29 cm-K. (K is degrees Kelvin).   Convert the wavelength from part A into a frequency. The product of wavelength and frequency for electromagnetic radiation is a constant, the speed of light (c), 3 x 10^10 cm/s.
Hi, I just need help with Part 2 of 4 please. The answer I submitted of 4.592 × 1010 was not correct even in real number form and scientific e notation form.
1.1) In a star's core the average mass number for ions which are not hydrogen or helium is 10. The mass fractions of hydrogen is 0.60, of helium is 0.38, and all other elements is 0.02. Calculate the average ion mass in units of mH. 1.2) Explain two assumptions behind the Kelvin-Helmholtz timescale. 1.3) In the outer core of a massive star the temperature is 108 K. The mean particle weight is u = 0.62. Calculate the density of this region if the radiation pressure is equal to the thermal pressure. 1.4) For temperatures around 1.5 x 10' K in a stellar core, describe why it is hydrogen instead of heavier ions which undergo fusion. Also, when the temperature is higher, describe why higher mass ions can undergo fusion. 1.5) Describe two possible causes of convective instability in the outer regions of a low mass star.

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EBK THE COSMIC PERSPECTIVE

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