

The Sun
Presentation
•
Science
•
6th - 8th Grade
•
Practice Problem
•
Medium
+1
Standards-aligned
Barbara White
Used 9+ times
FREE Resource
9 Slides • 9 Questions
1
The Sun
Middle School
2
Learning Objectives
Identify the main layers of the Sun's interior and atmosphere.
Describe the process of nuclear fusion in the Sun's core.
Explain the key features observed on the Sun's surface, such as sunspots and solar flares.
Differentiate between the photosphere, chromosphere, and corona.
3
Key Vocabulary
Nuclear Fusion
The process where hydrogen atoms combine to form helium, releasing vast amounts of energy.
Photosphere
The visible layer of the Sun's atmosphere that we perceive as the star's surface.
Corona
The outermost layer of the Sun's atmosphere, which is visible during a total solar eclipse.
Sunspots
Temporary, dark, and cool areas on the Sun's surface caused by its magnetic field.
Solar Flare
A sudden and explosive release of magnetic energy that erupts powerfully into space.
4
What is the Sun?
The Sun is a Yellow Dwarf star at the center of our solar system.
It is made of hydrogen and helium and produces energy by nuclear fusion.
Its surface temperature is about 5,778 K and it is 4.6 billion years old.
About one million Earths could easily fit inside the Sun's enormous sphere.
5
Multiple Choice
The Sun's energy is a result of nuclear fusion, where hydrogen combines to form which other element?
Oxygen
Carbon
Helium
Nitrogen
6
The Sun's Interior
The core is where the Sun's energy is made by nuclear fusion.
Temperatures of 15 million degrees fuse hydrogen atoms into helium.
Energy moves through the radiation zone as electromagnetic radiation.
In the convection zone, hot gases rise and cool gases sink.
If fusion stopped, the Sun’s core would lose outward pressure, causing the outer layers to collapse inward under gravity.
7
Multiple Choice
In which layer of the Sun's interior does the process of nuclear fusion take place?
Convection Zone
Radiation Zone
Core
Photosphere
8
The Sun's Atmosphere
Photosphere
The photosphere is the inner layer of the Sun's atmosphere.
It is the part we see as the visible surface.
This layer of gas is thick enough to be visible.
Chromosphere
The chromosphere is the middle layer of the Sun's atmosphere.
It appears as a reddish glow during a total eclipse.
Its name comes from 'chroma,' which means color.
Corona
The corona is the outer layer of the Sun's atmosphere.
It looks like a white halo around the Sun.
It is only visible during a total solar eclipse.
9
Multiple Choice
Which layer of the Sun's atmosphere is only visible as a reddish glow during a total solar eclipse?
Photosphere
Chromosphere
Corona
Convection Zone
10
Features on the Sun
Sunspots
These are dark areas of gas on the Sun's surface.
They are significantly cooler than the gases that surround them.
Their count often changes, following an eleven-year cycle.
Prominences
These are huge, bright loops of gas anchored to the photosphere.
They can often extend far out into the Sun's corona.
Prominences frequently connect different parts of various sunspot regions.
Solar Flares & Wind
A solar flare is a sudden eruption of magnetic energy.
These events increase the continuous stream of the solar wind.
Solar wind particles from the corona cause auroras on Earth.
11
Multiple Choice
What are the dark, cooler areas on the Sun's surface that vary in number over an 11-year cycle?
Prominences
Solar Flares
Sunspots
The Corona
12
Common Misconceptions About the Sun
Misconception | Correction |
|---|---|
The Sun is on fire. | The Sun produces energy through nuclear fusion, not by burning. |
The Sun does not move or rotate. | It rotates on its axis and orbits the center of the Milky Way. |
Sunspots are permanent features. | Sunspots are temporary and follow a cycle of about 11 years. |
The corona is cooler than the Sun's surface. | The corona is much hotter than the visible surface, reaching millions of degrees. |
13
Multiple Choice
How does the movement of gas in the convection zone help transfer energy in the Sun?
It bounces energy from atom to atom.
Hot gases rise to the surface, cool, and then sink, creating a current.
It fuses hydrogen into helium to release energy.
It blocks energy from escaping the core for thousands of years.
14
Multiple Choice
Why can the chromosphere and corona typically only be seen during a total solar eclipse?
Because they are colder than the rest of the Sun.
Because the photosphere is so bright that it normally outshines them.
Because they only exist during an eclipse.
Because they are located in the Sun's core.
15
Multiple Choice
A scientist observes a sudden, powerful eruption from the Sun that lasts only a few minutes. This event is followed by an increase in auroras on Earth. What feature did the scientist most likely observe?
A sunspot, because it is a cooler region on the surface.
A prominence, because it is a long-lasting loop of gas.
A solar flare, because it is a brief, energetic eruption that increases solar winds.
The corona, because it is the outermost layer of the atmosphere.
16
Multiple Choice
If the process of nuclear fusion in the Sun's core were to stop, what would be the immediate effect on the outer layers?
The convection zone would immediately become hotter.
The outer layers would quickly begin to collapse inward due to gravity.
Solar flares would become more frequent.
The photosphere would become brighter instantly.
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Summary
The Sun is a yellow dwarf star that creates energy through nuclear fusion.
Its interior contains the core, radiation zone, and convection zone.
The Sun's atmosphere includes the photosphere, chromosphere, and corona.
Solar wind is a stream of particles from the Sun causing auroras.
18
Poll
On a scale of 1-4, how confident are you about the concepts covered in today's review?
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The Sun
Middle School
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