Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 16, Problem 9CC
To determine
The output from carefully monitoring the Sun’s vibrations.
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An astronomer discovers a star that has a peak wavelength of 617 nm. Determine the peak frequency and the temperature of the star's surface.
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Universe
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- What is the temperature of a star whose maximum light is emitted at a wavelength of 290 nm?arrow_forwardA typical wavelength of infrared radiation emitted by your body is 25 mm (2.5 × 10−2 m). Show that the energy per photon of such radiation is about 8.0 × 10−24 J.arrow_forwardFind the power per unit area radiated from the sun’s surface in the wavelength range 600.0 to 605.0 nm.arrow_forward
- Which one of the following is true regarding the energy of a photon? It depends upon the intensity. It depends upon its amplitude. It depends upon its frequency. It depends upon its velocity.arrow_forwardThe intensity of light from the Sun reaching the surface of the Earth is 1.36 kWm^−2. Assume thatthe radius of the Sun is 6.96×10^8m and the Earth to Sun distance is 1.5×10^11m. Calculate: (a) The temperature at its surface and the wavelength of its strongest radiation. (b) The total power radiated by the Sun.arrow_forward14. Which number is closest to the frequency of a photon with a wavelength of 5.0x10-7 m? a. 1.5x102 s-1. b. 1.7x10-15 s-1. c. 6.0x1015 s-1. d. 6.0x1014 s-1.arrow_forward
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