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Foundations of Astronomy (MindTap ...

14th Edition
Michael A. Seeds + 1 other
Publisher: Cengage Learning
ISBN: 9781337399920

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BuyFindarrow_forward

Foundations of Astronomy (MindTap ...

14th Edition
Michael A. Seeds + 1 other
Publisher: Cengage Learning
ISBN: 9781337399920
Chapter 8, Problem 8RQ
Textbook Problem
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How are granules and supergranules alike? How are they different?

To determine

The alike and difference between the granules and super granules.

Explanation of Solution

The granulation is the surface effects of the convection. There is several examples of evidence for the granulation. The time period of granulation is 1020mins. Each period it will fade, shrinking and replaced by new granulation.

We can see the hot elements moving outward from the center of the sun and the cooler elements moving towards the center of the sun when the convection is present

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Chapter 8 Solutions

Foundations of Astronomy (MindTap Course List)
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Ch. 8 - What heats the chromosphere and corona to maintain...Ch. 8 - Why does hydrogen, which is abundant in the Suns...Ch. 8 - What is the shape of the heliopause? What...Ch. 8 - How are astronomers able to explore the layers of...Ch. 8 - Energy can be transported by convection,...Ch. 8 - What evidence can you give that sunspots are...Ch. 8 - When in the cycle does the maximum number of...Ch. 8 - How does the Babcock model explain the sunspot...Ch. 8 - How is meridional flow related to the Suns...Ch. 8 - Meridional is derived from meridian. Look up the...Ch. 8 - What does the spectrum of a prominence reveal?...Ch. 8 - How do prominences affect Earth?Ch. 8 - How can solar flares affect Earth?Ch. 8 - Which has a more tightly bound nucleus, uranium or...Ch. 8 - Why does nuclear fusion require high temperatures...Ch. 8 - Why does nuclear fusion in the Sun occur only near...Ch. 8 - Four protons are combined in the proton-proton...Ch. 8 - Give an example of a charged subatomic particle...Ch. 8 - Examine the elemental abundances for the solar...Ch. 8 - How can astronomers detect neutrinos from the Sun?Ch. 8 - How did neutrino oscillation affect the detection...Ch. 8 - How Do We Know? How do confirmation and...Ch. 8 - How Do We Know? What does it mean when scientists...Ch. 8 - The radius of the Sun is 0.7 million km. What...Ch. 8 - What fraction of the Suns interior is the core?...Ch. 8 - The smallest detail visible with ground-based...Ch. 8 - What is the angular diameter of a star the same...Ch. 8 - If a sunspot has a temperature of 4200 K and the...Ch. 8 - How many watts of radiation does a 1-meter-square...Ch. 8 - If a sunspot has a temperature of 4200 K and the...Ch. 8 - The radial velocity of a granules center is found...Ch. 8 - Gusts of the solar wind travel as fast as 1000...Ch. 8 - If the Sun rotates once every 24.5 days at the...Ch. 8 - How much energy is produced when the Sun coverts 1...Ch. 8 - How much energy is produced when the Sun converts...Ch. 8 - A 1-megaton nuclear weapon produces about 4 1015...Ch. 8 - A solar flare can release 1025 J. How many...Ch. 8 - The United States consumes about 2.5 1019 J of...Ch. 8 - Use the luminosity of the Sun (the total amount of...Ch. 8 - The diameter of the Sun is 109 times the diameter...Ch. 8 - Arrange the following objects in order of...Ch. 8 - Whenever there is a total solar eclipse, you can...Ch. 8 - Look at Figure 8-3. To what height and which...Ch. 8 - Refer to Figure 7-8a and Figure 8-3. What kinds of...Ch. 8 - Refer to labels C, F, and G in the solar spectrum...Ch. 8 - The two images here show two solar phenomena. What...Ch. 8 - This image of the Sun was recorded in the extreme...

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