UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
11th Edition
ISBN: 9781319278670
Author: Freedman
Publisher: MAC HIGHER
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Chapter 16, Problem 55Q
To determine
The effect which occurs if someone is observing the Sun. Also, describe the preclusion taken by the astronomers to overcome such effect.
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From which atmospheric layer of the Sun did the photons originate that resulted in sunburn? How do you know?
Which of the following layers of the Sun can be seen with some type of telescope? Consider all forms of light, but do not consider neutrinos or other particles. (Give ALL correct answers in alphabetical order, i.e., B, AC, BCD...)A) Corona.B) Photosphere.C) Radiation Zone.D) Chromosphere.E) Convection Zone.F) Core.
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Chapter 16 Solutions
UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
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- Describe the two main ways that energy travels through the Sun.arrow_forwardStep-by-step, explain how energy flows from the center of the Sun to Earth.arrow_forwardThe radius of the Sun is 0.7 million km. Examine Figure 7-3 to estimate the thickness of the chromosphere. What fraction of the Sun’s radius is taken up by the chromosphere?arrow_forward
- A friend who has not had the benefit of an astronomy course suggests that the Sun must be full of burning coal to shine as brightly as it does. List as many arguments as you can against this hypothesis.arrow_forwardWhat do measurements of the number of neutrinos emitted by the Sun tell us about conditions deep in the solar interior?arrow_forwardWhat it the Zeeman effect and what does it tell us about the Sun?arrow_forward
- Why do sunspots look dark?arrow_forwardDescribe how energy makes its way from the nuclear core of the Sun to the atmosphere. Include the name of each layer and how energy moves through the layer.arrow_forwardIf a sunspot has a temperature of 4200 K and the average solar photosphere has a temperature of 5800 K, how many times brighter is a square meter of the photosphere compared to a square meter of the sunspot? (Hint: Use the Stefan-Boltzmann law in Reasoning with Numbers 6-1.)arrow_forward
- Make a sketch of the Sun’s atmosphere showing the locations of the photosphere, chromosphere, and corona. What is the approximate temperature of each of these regions?arrow_forward1) What is thermal equilibrium? Is the Sun in thermal equilibrium? How do we know this? 2) In order to maintain thermal equilibrium, how much energy must the Sun generate every second?arrow_forwardUsing the concept of hydrostatic equilibrium, explain why the Sun does not collapse under the weight of its own gravity.arrow_forward
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