
The Sun
Presentation
•
Science
•
7th - 8th Grade
•
Practice Problem
•
Medium
Standards-aligned
Logan Oliver
Used 388+ times
FREE Resource
17 Slides • 8 Questions
1
The Sun
Structure, Atmosphere, and Features
2
Interior of the Sun
The Sun's Interior is composed of three main sections:
Core
Radiation Zone
Convection Zone
3
The Core
The Sun produces an A LOT of energy in the core through nuclear fusion
Nuclear fusion occurs when HYDROGEN atoms combine to form HELIUM
This process requires extremely high temperatures and pressure
4
The Radiation Zone
The energy produced in the Sun's core moves outward through the radiation zone
This is a region of very tightly packed gas where energy moves mainly in the form of electromagnetic radiation
This zone is so dense that it can take over 100,000 years for the energy to move through it
5
The Convection Zone
This is the outermost layer of the Sun's interior
Hot gases rise from the bottom of the convection zone and slowly cool as they approach the top
Cooler gases sink, forming loops of gas that move energy toward the Sun's surface
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7
Multiple Choice
What layer of the Sun's interior produces the energy?
Convection Zone
Core
Radiation Zone
Corona
8
Multiple Choice
In the convection zone, ______ gas rises and ______ gas sinks.
hotter, cooler
cooler, hotter
9
Multiple Choice
The sun produces energy through what process?
Fission
Fusion
Photovoltaic cells
Photosynthesis
10
The Sun's Atmosphere
The Sun's atmosphere is composed of three main sections:
Photosphere
Chromosphere
Corona
11
The Photosphere
Inner layer of the Sun's atmosphere
This layer of gas is thick enough to be visible and is considered the surface layer
When you look at an image of the Sun, you are looking at the photosphere
12
The Chromosphere
Middle layer of the Sun's atmosphere
This layer is seen as a reddish glow around the photosphere
Can only be seen at the start and end of a total eclipse
The Greek word chroma means "color" so the chromosphere is really the "color sphere"
13
The Corona
Outer layer of the Sun's atmosphere
Looks like a white halo around the sun
Only seen during an eclipse
Extends into space for millions of kilometers
Corona means "the crown" in Latin
14
Multiple Choice
Which layer of the Sun's atmosphere is only seen at the beginning and end of an eclipse?
Photosphere
Corona
Chromosphere
Radiation Zone
15
Fill in the Blanks
Type answer...
16
Features of the Sun
Sunspots
Prominences
Solar flares
Solar wind
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Sunspots
Areas of gas on the Sun's surface that are colder than the gases around them
Colder gases don't give off as much light
Can be larger than the Earth
The # of sunspots varies in a regular cycle, with the most appearing about once every 11 years
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Prominences
Huge loops of gas that often link different parts of sunspot regions
These loops of gas are anchored to the photosphere and extend to the corona
Can last for months
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Solar Flare
A release of magnetic energy that heats gas in the Sun's atmosphere and causes an eruption into space
Typically lasts for a few minutes
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Solar Winds
Streams of electrical particles from the Sun
Solar flares can increase the amount of particles
Earth's magnetic field blocks the majority of solar winds except on the North and South Poles
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Solar Winds cont.
At the poles, the particles create electric currents that cause gas in the atmosphere to glow (Aurora Borealis a.ka. Northern Lights)
Worst case scenarios: too many particles entering the atmosphere can cause magnetic storms and blackouts
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23
Multiple Choice
Large eruptions of heated gas from the Sun's surface are called
Prominences
Solar winds
Sunspots
Solar flares
24
Multiple Choice
The corona sends out a stream electrical particles called the
Solar flares
Solar winds
Sunspots
Prominences
25
Fill in the Blanks
Type answer...
The Sun
Structure, Atmosphere, and Features
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