21ST C ASTRO EBOOK+SW5=SS+VGCRD+LEARN/DO
21ST C ASTRO EBOOK+SW5=SS+VGCRD+LEARN/DO
6th Edition
ISBN: 9780393870152
Author: PALEN
Publisher: Norton, W. W. & Company, Inc.
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Chapter 14.3, Problem 14.3CYU
To determine

The reason for sharp appearance of sun’s surface in visible light.

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The Sun's photosphere is a. the central region where the Sun originates b. the part of the Sun which the light comes that we see when we look at the Sun with our eyes c. the hottest region of the Sun d. the outermost layers of the Sun's atmosphere e. the first region you would come to when leaving the core
The capture of too few solar neutrinos by Davis in the solar neutrino experiment   a. can be explained if the sun is not undergoing thermonuclear fusion of hydrogen in its core.   b. indicates that the sun’s core is much cooler than expected.   c. indicates that the sun’s core is much hotter than expected.   d. indicates that the sun’s core is convective.   e. is explained by none of the above.
62. Pressure of the Photosphere. The gas pressure of the photosphere changes substantially from its upper levels to its lower levels. Near the top of the photosphere, the temperature is about 4500 K and there are about 1.6 x 1016 gas particles per cubic centimeter. In the middle, the temperature is about 5800 K and there are about 1.0 x 10" gas particles per cubic centimeter. At the bottom of the photosphere, the temperature is about 7000 K and there are about 1.5 × 10" gas particles per cubic centimeter. Use the ideal gas law (Mathematical Insight 14.2) to compare the pressures of each of these layers; explain the reason for the trend that you find. How do these gas pressures compare with Earth's atmospheric pressure at sea level?
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